The galaxy presents as a single, centrally concentrated object with a smooth morphology. It exhibits a roughly circular shape, lacking any distinct spiral arms, bars, or other prominent features typically associated with disk galaxies. The galaxy's color profile is relatively uniform, trending towards the redder end of the spectrum. This redder hue suggests a population dominated by older stars, indicative of a galaxy where star formation is largely quiescent. There is no apparent indication of ongoing mergers or tidal disturbances that would otherwise disrupt the smooth appearance. The galaxy appears isolated, without any nearby companions or signs of interaction. The light is most concentrated at the center, with a gradual decrease in surface brightness towards the outer edges of the galaxy.
