This galaxy presents a largely smooth morphology, suggesting it is likely an elliptical galaxy. The central region exhibits a high degree of sphericity with a concentrated luminosity profile. The light distribution appears relatively uniform and undisturbed, showing little evidence of spiral arms or significant dust lanes. There may be some indication of minor disturbances in the outer halo, but this is not definitive. The galaxy exhibits a color gradient, appearing more red in the core and somewhat bluer toward the outskirts. The overall color index implies that the galaxy's stellar population is likely dominated by older, redder stars. No merging companions or major tidal features are readily apparent.
