The galaxy presents a primarily smooth morphology, indicative of a likely elliptical or lenticular type. It exhibits a concentrated central bulge that fades gradually into the surrounding halo. The overall color appears to be somewhat redder, suggesting a population of older stars and a lower rate of on-going star formation. There is no apparent spiral structure or well-defined disk visible. The galaxy appears relatively undisturbed, without major signs of recent mergers or tidal interactions, though there might be some minor disturbances within the galaxy due to interactions in the past. The shape is tending towards a more flattened profile but not extremely so.
