The galaxy presents as a primarily smooth and concentrated elliptical morphology. There's a notable color gradient, with a redder, possibly older stellar population concentrated towards the central bulge region, suggesting a more evolved system. The outer regions appear slightly bluer, potentially indicating some ongoing, though likely minimal, star formation activity. The shape is predominantly round, with a very slight elongation. There's no evidence of major disturbances or merging events, although a very faint, almost imperceptible asymmetry might suggest a past minor interaction. Overall, the galaxy is relatively compact and possesses no obviously prominent disk features. The integrated light profile is dominated by the bulge.
