This galaxy appears to be a spiral galaxy, viewed at an oblique angle. It exhibits a moderate degree of central concentration, with a relatively smooth light distribution, but the presence of irregularities suggest potential disk-like features. There appears to be a faint, extended disk that is slightly more apparent on one side, potentially indicating warping or tidal interactions.

The overall color is moderately blue, especially towards the center, potentially indicating ongoing star formation. There is some indication of minor dust lanes, but without better resolution, it is difficult to determine how pervasive they are. The shape is elongated, suggesting a possible S0 type. There are no signs of a clear galactic merger, but subtle disturbances are noted in the shape, giving it the suggestion of minor interaction with another galaxy.
