This galaxy presents a generally elliptical morphology, though some subtle features suggest the presence of a disk. The central bulge appears prominent and exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Moving outward from the core, the galaxy displays a diffuse halo with a bluer color, which could be associated with ongoing or recent star formation activity. 

There appears to be some asymmetrical structure in the outer regions, suggesting possible gravitational interaction or past mergers. The galaxy is relatively smooth in appearance.
