The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing almost spheroidal. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region. The outer regions are fainter and subtly more bluish. No distinct spiral arms or prominent dust lanes are visible, indicating a lack of significant recent star formation. The overall morphology appears undisturbed, with no obvious signs of tidal interactions or ongoing mergers.
