The galaxy presents as a single, relatively smooth and rounded object. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The color profile suggests a population of older stars, evidenced by the yellow-red hue of the central bulge, though some bluer regions are detectable surrounding the core. The light appears generally uniform and lacks any pronounced spiral arm structure or significant dust lanes. There are no obvious signs of ongoing or recent major merger events. Overall the galaxy appears consistent with an elliptical morphology.
