The galaxy appears as an elliptical shape, elongated with a noticeable cigar-like form. The light distribution suggests a smooth, concentrated central bulge that fades gradually outward. The color profile indicates an aging stellar population, with a dominant reddish-yellow hue in the core, and a slight hint of bluer components at the periphery, which may imply younger stars or star forming regions in the outer reaches. The galaxy seems undisturbed, showing no obvious signs of major mergers or tidal disruptions, but there may be minor asymmetries visible. The general morphology suggests it is a relatively evolved system with ongoing, moderate star formation activity.
