The galaxy appears to be an elliptical galaxy. It exhibits a generally smooth, centrally concentrated light distribution, lacking prominent spiral arms or a well-defined disk structure. The morphology is predominantly spheroidal, with a slight elongation. Color gradients are present. The core region appears yellow-orange, potentially indicative of an older stellar population. The outer regions show a bluer tinge, indicating possible recent, albeit limited, star formation. There is no significant evidence of tidal features, major mergers, or strong interactions with other galaxies. A slight asymmetry in the outer isophotes suggests the possibility of a minor disturbance.
