The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. The light profile appears centrally concentrated with a gradual decrease in intensity outwards, lacking distinct spiral arms or prominent features associated with disk galaxies. The primary color is yellowish, suggesting a relatively older stellar population with fewer hot, young stars. There is no visible evidence of active star formation regions. The overall morphology indicates a relaxed system with no signs of significant recent mergers or tidal disturbances, though there may be minor asymmetries suggesting a past interaction. The roundness of the galaxy indicates it is likely an E0-E3 type elliptical.