The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing moderately elongated rather than perfectly spherical. The core region is significantly brighter and more yellow-hued than the surrounding area, suggestive of an older stellar population dominating the center. Fainter, less defined extensions or a diffuse halo are observed extending from the main body, exhibiting a bluer color. There are no obvious indications of strong spiral arm structures or significant dust lanes. The overall structure appears relatively undisturbed, without any major signs of ongoing mergers or tidal disruptions. There are some subtle asymmetries visible within the extended halo, though these are slight. The galaxy is likely a passively evolving system.
