The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The outer regions show a gradual decrease in luminosity, with a faint, diffuse halo extending beyond the central region. There is a subtle color gradient from the core to the outer edges, with the periphery exhibiting a slightly bluer tinge compared to the core. No distinct spiral arm structures or significant dust lanes are discernible. Overall, the galaxy's morphology indicates a system dominated by older stars with minimal ongoing star formation. There is no evidence of any major mergers or significant tidal disturbances.
