The galaxy presents as a centrally concentrated object with a relatively smooth appearance. The light distribution appears generally round, with minimal elongation. There is a distinct bright central region, possibly indicative of a galactic nucleus or a high concentration of stars in the core. The overall color is a cool hue, possibly enriched in younger stellar populations. The outer regions of the galaxy appear diffuse and less defined compared to the central bulge. There is no strong evidence of spiral arms or significant disk structures. No obvious signs of tidal disturbances or ongoing mergers are visible.
