The galaxy appears as a centrally concentrated object with a smooth light distribution. The central region exhibits a bright, compact core, suggesting a high stellar density. The galaxy appears mostly featureless, with a gradual decrease in surface brightness moving outwards from the core. There are no apparent spiral arms, bar structures, or dust lanes visible in this image. The shape appears mostly elliptical in projection, although it is difficult to discern the exact ellipticity due to the limited resolution. There might be a faint, extended halo or envelope surrounding the central body. Based on the color profile, the galaxy seems to consist predominantly of older stellar populations, indicated by the slightly redder hue. No signs of major mergers or strong tidal disturbances are apparent, although subtle asymmetries cannot be ruled out.
