The galaxy appears as a relatively compact object with a smooth, elliptical morphology. The light distribution suggests a centrally concentrated structure, with a gradual decrease in surface brightness outwards. There is little to no evidence of spiral arms or a distinct disk component. The overall color is yellowish-orange, indicating a population of older stars and possibly significant dust content. There may be some minor asymmetry present, potentially indicating a past or ongoing minor interaction, but no significant tidal features or distortions are readily apparent. The galaxy appears to be relatively isolated within its immediate surroundings.
