The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, though it does display a slight disk-like structure when viewed edge-on. There is a noticeable color gradient, with the central bulge appearing more yellow or golden, indicative of an older stellar population. The outer regions of the galaxy appear slightly bluer, potentially suggesting the presence of younger stars or ongoing star formation, albeit at a relatively low rate. No major disturbances or merging features are readily apparent in the image, although subtle asymmetries may suggest minor interactions or past events.
