The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright, concentrated central bulge that graduates outwards to a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-orange hue dominating. There is little evidence of spiral arms or significant dust lanes within this image. The galaxy appears largely undisturbed, showing no obvious signs of tidal interactions or recent mergers. It exhibits a high degree of circularity in its overall shape.
