The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. The core is bright and yellowish-white, indicating an older stellar population. Fainter, reddish light extends outwards in a diffuse halo, suggesting the presence of older, redder stars in the outer regions. There is little evidence of spiral arm structure or significant dust lanes, supporting its classification as an elliptical galaxy. The overall shape appears close to round. There are no obvious signs of recent major mergers or tidal disturbances.
