The galaxy presents as an elliptical-like structure with a relatively smooth appearance, although subtle irregularities suggest possible interactions or internal disturbances. The object displays a generally concentrated light profile, with a brighter central region that gradually fades outwards. The galaxy exhibits a moderate degree of ellipticity; it is somewhere between round and elongated. Some patches of slightly bluer light may be associated with regions of ongoing star formation. These star forming regions could be due to the minor disturbances or mergers that are indicated by some of the irregularities in its form. There are some faint extensions or tidal features possibly indicative of past or ongoing interactions, but they are not strongly defined. Overall, the galaxy appears to be a relatively evolved system with a mix of smooth, spheroidal components and subtle features suggesting dynamical activity.
