The galaxy appears to be an elliptical type, characterized by a generally smooth and featureless morphology. The light distribution is concentrated towards the center, displaying a gradual decrease in surface brightness with increasing radial distance. The main body of the galaxy appears slightly elongated. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a color gradient, with the central region appearing more yellow, possibly indicating an older stellar population. The outer regions show a bluer tinge, which could indicate a younger, although not prominent, stellar population. There is no evidence of any major mergers or significant tidal disturbances.
