The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a gradual increase in luminosity towards its center. It has a noticeable central bulge which appears yellow, suggesting a population of older stars. The outer regions of the galaxy show a disk-like structure that isn't well defined, and appears to have a bluer hue, possibly indicating the presence of younger stars and ongoing star formation in the outer regions. There is some indication of minor disturbance in the form of subtle asymmetric features. The galaxy's overall shape leans toward a flattened spheroid, and its color gradient suggests a transition from an older stellar population in the core to a younger population in the outer regions, although the galaxy overall does not display prominent star formation.
