The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core region is bright and slightly yellowish, indicative of an older stellar population. The outer regions exhibit a gradual decrease in luminosity with a more reddish tint. There are only faint signs of spiral arms or significant substructure within the galaxy. The overall shape is more elongated than circular but without obvious signs of ongoing merger activity or strong tidal disturbances. There appears to be little to no active star formation.
