The galaxy presents as a relatively smooth, elliptical morphology. Its central bulge is luminous and exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions are less defined, with a subtle disk-like structure, although not sharply delineated. There is some indication of minor disturbances or tidal features in the fainter outer halo, which could be indicative of past interactions or mergers. Overall, the galaxy appears to be in a relatively quiescent state with little active star formation in the central regions, though there may be some in the outer reaches.
