The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. The galaxy has a generally rounded morphology, showing little evidence of a disk-like structure. There is no obvious indication of significant tidal features, major mergers, or strong disturbances within its structure. It presents a yellow-ish color, consistent with a population of older stars. Star formation appears to be occurring at a low rate. 
