The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge region with a gradual decrease in luminosity moving outwards. Color gradients are subtle, with a somewhat bluer hue toward the core, suggesting a concentration of younger, hotter stars, and a slightly redder tint on the outer edges, indicating an older stellar population. No distinct spiral arms or significant dust lanes are discernible. The galaxy exhibits no strong indications of major merger activity or tidal disturbances, appearing mostly undisturbed. It possesses moderate intrinsic brightness and a compact size. The overall morphology suggests an evolved system, likely dominated by older stars, but potentially with a pocket of recent or ongoing star formation activity in the nuclear region.
