The galaxy presents a largely smooth, elliptical morphology. It is highly concentrated with a bright, relatively small core that fades into a more diffuse halo. The color gradient suggests an older stellar population. The galaxy's smooth appearance does not exhibit signs of significant recent mergers or tidal disturbances. Although some minor irregularities are observable in the outer regions, no clear disk or spiral arm structures are visible. This galaxy appears to be a well-formed, mature system.
