The galaxy appears as a largely featureless, smooth elliptical or lenticular type system. Its overall shape is quite round. The core of the galaxy displays a concentration of light, potentially indicative of a supermassive black hole at the galaxy's center. The light profile gradually fades outward from the central region, lacking any distinct spiral arms, bars, or prominent dust lanes. The galaxy exhibits a yellowish-white hue, which suggest a stellar population dominated by older, redder stars. The galaxy does not seem to be undergoing any major merging activity or tidal disturbances.