The object presents as a single, relatively smooth and rounded galaxy. No spiral arm structure is readily apparent. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outward from the center. There is a slight elongation of the galactic shape but, overall, the galaxy appears largely spheroidal. There is no evidence of a pronounced disk or significant dust lanes. The galaxy appears to be relatively undisturbed, with no obvious signs of tidal interactions or ongoing mergers. The color profile suggests a population of older stars, with a redder hue observed. Minimal signs of active star formation are evident from the image.
