The galaxy presents as a relatively smooth, elliptical morphology. The light distribution is concentrated centrally, with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a yellow-white hue in its core, potentially indicating an older stellar population. Fainter, bluer regions appear to exist in the outer regions of the galaxy. There is no apparent spiral arm structure or significant dust lane features. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions.
