0238(=NGC4944): Curious disk structure, with two positive maxima of e4, separated by an intermediate area with negative e4, while e6 remains large. 0334(= NGC4934): Dusty galaxy with asymmetric and non concentric isophotes, probably an S. Classified S in GMP and S? in RC3. Inner ring giving a sharp peak of e4 = 0.12. 0421(= NGC4929): An envelope with strong twist, decreasing axis ratio, and disky isophotes is found. 0485: Inner ring and lens. 0504: Several shape coefficients differ from zero, which is evidence for irregular isophotes. Confirmed by visual inspection of the image. 0539: Inner ring and lens. 0591: There are uncertainties in the analysis of this roundish object. The profile follows the r^1/4^ law, while a bar-like twist of the inner isophotes is observed. 0661(= NGC4923): There is evidence for an inner embedded disk in this roundish elliptical with a very large and regular isophotal twist. 0694: This galaxy shows a large spheroid, surrounded by a disky envelope well above the extrapolated SuBr of the "bulge". 0718(=NGC4919): Inner ring and lens. 0857: Marginal evidence for a low-contrast bar. 0867: Uncertain analysis, due to the presence of low surface brightness fluctuations which may or may not be intrinsic to the galaxy. 0876(= NGC4906): There is evidence for an inner embedded disk. 1035(=RB167): The galaxy has an inner boxy structure and a disky envelope. The boxiness is attributed to a bar, slightly tilted within the disk. 1039(= NGC4889): A large cD galaxy with a very extended envelope. The field of the CCD was not sufficient to extend the analysis to low SuBr. 1050(=RB077): Strong blend with NGC 4889. It was measured after subtraction of a spheroidal image of the cD galaxy. 1065(=NGC4886): Blend with NGC 4889. 1115 (= RB 155): A dominant bar is surrounded by a roundish envelope. 1198 (=RB41): Companion to the West. 1204: Dust in the southern part of the disk of this North-South oriented galaxy. An S galaxy almost edge-on? 1214 (=RB 022): Marginal evidence for a bar in a lens. 1258 (=RB 026): The analysis is uncertain due to the halo of a very bright nearby star. 1277 (=RB 022): The large twist of the outer isophotes may be related to the halo of a very bright nearby star. 1300 (=RB 014): The large bulge looks like a bar along the major axis. 1378 (=NGC 4864): Uncertain analysis, due to a parasitic star 7 arcsec from the galaxian center. 1406 (=IC 3957): Our V frame would lead to the diE class, but this is contradicted by the R frame. A dust ring has been detected. 1414 (=IC 3955): This galaxy contains a small bulge at PA circa 70deg, then a large dominant bar at PA = 45deg, surrounded by a more roundish, strongly twisted envelope. S-shaped isophotes occur at the tips of the bar. It shows similarities with NGC 3414 (Michard 1994). 1507 (=NGC 4854): The bar is suspect, because the stellar images are elongated, but the KP 1608 data confirm its presence. 1524: Irregular isophotes. 1646: This galaxy presents noticeable asymmetries, but its luminosity profile deviates very little from the r^1/4^ law; doubtful classification. 1823 (=NGC 4842a): Marginal photometric evidence for a faint disk in this roundish galaxy, while e4 remains zero. 1828 (=NGC 4841b): Difficult analysis because it is a roundish galaxy in the halo of NGC 4841a. 1831 (=NGC 4841a): The large twist of the outer isophotes is uncertain, due to the difficulty of separating NGC 4841a and b. 1834 (=NGC 4840): The suspected bar is probably spurious (elongated stellar images). 1878(= NGC4839): The low average SuBr suggests that this galaxy is dominated by an extended disk. The galaxy is disky inside r_e_ and boxy outside. 2074: Very large twist of the nearly circular isophotes. 2134 (=NGC 4816): This giant elliptical has an extended envelope well above the r^1/4^ law relevant to the inner parts. 0733 (=RB 129): Data from a frame kindly provided by C. Lobo (Institut d'Astrophisique de Paris). 1039 (=NGC 4889): Global photometry cannot be obtained from small results for the integrated photometry. The total magnitude is underestimated. 1331 (=NGC 4865): This object shows a dust ring of circa 1" radius. 1883: This galaxy is a companion to a massive E, i.e. NGC 4839, so that its analysis refers to a limited radial extent. It is tempting to classify it amont the small boE's "satellites"; recognized as a specific group by Nieto & Bender (1989). 2109: This object is projected against the envelope of NGV 4816. 0884 (=IC 4040): Important dust pattern. 0969 (=RB 094): The bar is the dominant component. 0976 and 0989 (=MGC 4898b and a): A pair of overlapping early-type objects, with their centers about 6" apart. 1035 (=RB 167): The e4 coefficient oscillates between an inner negative value, tentatively associated with a bar, and an outer positive one. The values of e4 in Table 2a and 3 disagree only because they where not measured at the same isophote! 1039 (=NGC 4889): It is the eastern component of the famous pair of cD galaxies near the cluster center. It displays a very extended envelope. 1050 (=RB 077): It lies inside NGC 4889. A model of the giant galaxy was substracted from the frame, before measuring the companion. 1109 (=NGC 4883): This object displays a strongly twisted and asymmetric envelope. The morphological type is uncertain. 1115 (=RB 155): This object looks like a strong bar surrounded by a roundish envelope. e4 is >0 as the transition. 1177 (=RB 045): This evidence for a disk is marginal. 1181 (= RB 043): The isophotes in the envelope are strongly twisted compared to the main body of this small boE object, hence its classification as pec. This is reminiscent of NGC 4478 in the Virgo cluster. Our CCD TBL image does not confirm this twist. 1233 (= NGC 4874): It is the western component of the characteristic pair of cD galaxies in the Coma cluster (with NGC 4889). It displays an extended envelope, well above the r^1/4^ law, as extrapolated from the inner regions. 1258 (= RB 026): Difficult analysis, due to the halo of a very bright star. 1266 (= RB 234): The evidence for a disk is marginal. 1277 (= RB 022): Difficult analysis. due to halo of a very bright star. 1373 (= RB 268): This roundish galaxy has such a low effective SuBr that it is probably a disk dominated object. 1378 (= NGC 4864): A rather bright star 7 arcsec away from the galaxian center makes the isophotal analysis rather uncertain. 1414 (= IC 3955): See description in Seet. 5.1. 1458 (= IC 3949): Edge-on galaxy with an important dust pattern. 1489 (= RB 252): A strongly inclined SA0 with evidence for an f4-asymmetry. 1620 and 1623 (= NGC 4851): Pair of mildly overlapping galaxies. 1724: This is not one galaxy, but two overlapping galaxies with their nuclei about 3 arcsec apart. 1739: Doubtful case! e4 is clearly >0 only for a<3", i.e. in a range where it is uncertain. 1758: This object becomes roundish outwards. The envelope might be a disk with an unresolved spiral patterns or a spheroidal halo. The latter is less likely because of the large and consistent twist of the outer isophotes. 1844: Important ring-lens. 1687: Important dust pattern. 1778: An edge-on S0 with a clear f4-asymmetry. 2034: Important dust pattern. This object might be an Sa. D16: This galaxy is asymmetric and of low SuBr with evidence for dust. FW10: A disk is detected at large radii. NGC 4692: This galaxy has been classified as unE from our CCD image, at variance with the present determination. The twist of the PA is uncertain for this roundish galaxy. FW2: The twist of the PA is uncertain. D3: An edge-on galaxy with a clear f4-asymmetry. anon04: Galaxy interacting with supp08. D11: An edge-on galaxy with a clear f4-asymmetry. D10: This galaxy has a ring similar to that of NGC 4215. FW9: This unE shows an outer disk. D12: An edge-on SA0 with a clear f4-asymmetry. supp01: The PA twist is uncertain. suppO6: Dust detected. D14: A low SuBr dusty galaxy. supp08: It is interacting with anon04 D6: A spiral, judging from the asymmetry. supp09: Asymetric and dusty galaxy. supp12: This galaxy is not FW3.