The galaxy presents as a concentrated, yellowish-white elliptical shape. It appears relatively smooth in texture, with no apparent spiral arm structures or prominent dust lanes visible. The core is a bright, somewhat compact region that gradually fades into a more diffuse halo. While there are no obvious signs of major disruption or ongoing merger events, there may be minor disturbances in the outer edges, suggesting possible past interactions or accretion events. The overall morphology suggests an evolved galaxy, likely with a considerable population of older stars.
