The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology with a moderate degree of roundness. There is a suggestion of a disk component, although it does not dominate the overall structure. A minor disturbance or interaction cannot be ruled out, indicated by slight asymmetry or subtle features.

Color gradients are apparent, with a more yellowish core, suggestive of an older stellar population, gradually transitioning to bluer outer regions, perhaps indicative of ongoing star formation. The central bulge is significant, and the overall luminosity suggests a massive system.
