The galaxy appears to be a relatively smooth, elliptical-like system. There is a distinct concentration of light toward the center, suggesting a central bulge. The color profile indicates an aging stellar population, with a yellowish hue dominating the core region. Fainter, bluer regions are observed in the outer parts of the disk, suggesting some recent star formation. The overall morphology appears undisturbed, with no obvious signs of major mergers or tidal disruptions, though a slight asymmetry may indicate a minor interaction or internal activity. The galaxy's general roundness implies a relatively high degree of rotational support or that it may be an elliptical galaxy.
