| ID | A | C | G | M20 |
| (1) | (2) | (3) | (4) | (5) |
| NGC 0628 | 0.31 | 0.31 | 0.45 | -1.54 |
| NGC 3031 | 0.18 | 0.42 | 0.57 | -2.33 |
| NGC 3049 | 0.27 | 0.50 | 0.76 | -2.29 |
| NGC 3184 | 0.27 | 0.32 | 0.53 | -1.45 |
| NGC 3521 | 0.29 | 0.61 | 0.70 | -2.41 |
| NGC 3938 | 0.34 | 0.48 | 0.66 | -1.83 |
| NGC 4536 | 0.25 | 0.34 | 0.50 | -1.50 |
| NGC 4569 | 0.21 | 0.50 | 0.65 | -1.88 |
| NGC 4579 | 0.14 | 0.58 | 0.70 | -2.48 |
| NGC 4625 | 0.36 | 0.71 | 0.74 | -1.81 |
| NGC 4725 | 0.24 | 0.40 | 0.54 | -2.41 |
| NGC 5055 | 0.15 | 0.52 | 0.63 | -2.13 |
| NGC 5194 | 0.35 | 0.26 | 0.47 | -1.42 |
| NGC 5713 | 0.32 | 0.65 | 0.83 | -2.13 |
Notes. Column (1):
object ID; Col. (2): asymmetry index; Col. (3):
concentration index;
Col. (4): Gini coefficient; Col. (5): M20
index.
We could not obtain reliable measurements of the photometric parameters
of NGC 3621, NGC 4236, NGC 2976 and
NGC 7331 because of the large number of stars and artifacts on
the images, therefore they are not used in our analysis.
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