The galaxy presents a morphology suggestive of an elliptical or lenticular type, exhibiting a primarily smooth, centralized structure with a notable lack of distinct spiral arms or significant dust lanes. The overall shape appears roughly circular, tending toward round rather than elongated. There may be a faint suggestion of a disk component embedded in the halo or bulge, but the smoothness of the light distribution dominates.

Color variations within the galaxy are subtle, with a central core displaying a yellowish hue indicative of an older stellar population, potentially containing red giant stars and fewer young, hot stars. The outer regions exhibit a shift towards slightly bluer shades, possibly indicative of a small amount of ongoing star formation or a different stellar composition in these areas. There are irregularities on the right side that also look like they are bluer in color. The light from the galaxy fades off gradually at its edges, merging into the background sky.

Visually, the galaxy appears to be undergoing or to have undergone some form of gravitational interaction or disturbance, possibly a merger with a smaller galaxy or tidal effects from a past encounter.
