The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a central bulge that dominates its overall structure, with a gradual decrease in luminosity extending outwards. The galaxy appears generally rounded, showing a slight elongation but lacking any prominent spiral arm structure or distinct features suggesting a recent major merger event. There may be some indication of minor disturbances, possibly resulting from a minor merger or tidal interaction, but these features are not as pronounced.

The galaxy's color appears to be redder towards the center, which could indicate an older stellar population dominating the bulge, while the outer regions show a hint of bluer light, suggesting some recent star formation activity, although not at an exceptionally high rate.
