The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology and a centrally concentrated light profile. It is nearly circular in shape. The galaxy exhibits a slight color gradient, transitioning from a yellowish central bulge to a bluer outer halo. This color difference may indicate variations in stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars more prevalent in the outer regions. There is no evidence of spiral arms, a bar, or significant dust lanes. The galaxy appears isolated, without any signs of tidal interactions or mergers. The light distribution appears relatively even, suggesting a lack of recent star formation. The overall impression is that of a relatively evolved, quiescent galaxy dominated by an older stellar population.
