The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a higher surface brightness, gradually decreasing outwards. There is a lack of discernable spiral arm structure or prominent dust lanes. The overall color appears slightly redder, suggesting a stellar population dominated by older stars. The galaxy appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. Minor disturbances cannot be ruled out, but the primary impression is one of a settled, spheroidal system.
