The galaxy presents an overall smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a fairly regular, round shape, with only a slight elongation. There is no apparent spiral arm structure or significant disk component visible. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color profile indicates a redder core region, transitioning to a slightly bluer halo. No signs of active galactic nuclei are apparent in this image. The overall appearance suggests a relatively evolved system, potentially quiescent in terms of star formation activity, and may have undergone some kind of minor merging event with its smaller neighbour.
