The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing more rounded than elongated. A color gradient is discernible, with a yellowish-orange hue dominating the central region, potentially indicative of an older stellar population. The outer regions show hints of a bluer color, hinting at the presence of younger stars or ongoing, albeit limited, star formation. There are no obvious signs of significant tidal disturbances or major mergers in its recent history based on this image. The overall morphology suggests a galaxy that is relatively undisturbed and potentially evolved.
