The galaxy presents as a somewhat elliptical or disk-like structure, exhibiting a relatively smooth overall appearance. The central region is characterized by a bright, concentrated luminosity, which gradually fades towards the outer edges. A slight color gradient is discernible, with the core appearing more yellow, possibly indicating an older stellar population, while the outer regions exhibit a bluer tint that is less distinct, suggesting the presence of younger stars or ongoing star formation, though at a potentially low rate. There is no strong evidence of spiral arms, bar features, or significant morphological disturbances; it appears to be a relatively settled system.
