The galaxy presents as a concentrated, centrally brightened system, appearing nearly circular in projection. It exhibits a smooth light distribution, with no immediately discernible spiral arm structure or prominent dust lanes. The color profile suggests a population of older stars, with a yellow-orange hue dominating the central region, transitioning to a slightly bluer, though still muted, color in the outer regions. There are no obvious signs of a recent major merger or significant tidal disturbances, although some subtle irregularities in the outer halo suggest possible minor interactions or past accretion events. The overall morphology is consistent with that of an elliptical galaxy, perhaps with a small disk component. Star formation is likely present but at a low rate.
