The galaxy presents as a largely featureless elliptical or lenticular structure. It exhibits a smooth, centrally concentrated light profile, with the luminosity decreasing gradually from the core outwards. The color gradient suggests an older stellar population, with a yellowish-white hue dominating the central region, indicative of evolved stars. There are subtle color variations in the outer regions, hinting at the presence of some younger, bluer stars, though the overall star formation rate appears to be relatively low. The overall shape is moderately elongated. There's no evidence of significant dust lanes, spiral arms, or tidal features to indicate a recent major merger event. The galaxy seems relatively undisturbed.
