The galaxy presents as a centrally concentrated, relatively smooth object with a generally elliptical morphology. A bright, slightly diffuse core is apparent, surrounded by a more extended, fainter halo. The color profile suggests a mix of stellar populations, with the core showing a tendency towards slightly bluer hues compared to the more extended, reddish halo. There is a subtle suggestion of asymmetry or a minor disturbance in the halo region on one side, potentially indicating an interaction or merger event in its past. The overall appearance is indicative of a galaxy with a significant spheroidal component, consistent with an early-type or an aging spiral galaxy.
