The galaxy presents as an elliptical or lenticular type based on its smooth, rounded morphology and lack of discernible spiral arms. There is a bright central bulge, possibly indicating a significant supermassive black hole and a high concentration of older stars. The outer regions appear more diffuse, fading into the background sky. The overall color is yellowish, suggesting a stellar population dominated by older, redder stars, although the blue magnitude suggests the presence of some younger stars. Faint disturbances may be present within the extended halo, indicating potential past mergers or tidal interactions, yet overall the system appears relatively relaxed and evolved. 
