The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile. The core region is bright and intense, with a gradual decrease in brightness towards the outer edges, suggesting an older stellar population dominating. The overall color appears somewhat red-tinged, potentially indicative of evolved stars and/or dust obscuration. The galaxy seems to have a fairly symmetrical morphology without any obvious signs of spiral arms or strong tidal disturbances. There is no evidence of a prominent disk component.
