The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-spherical morphology, displaying a high degree of circularity. There is no clear evidence of spiral arms or a prominent disk structure. Some minor disturbances, like a slight bulge or tidal feature, may be present but the signal is low and no major mergers or significant distortions are visible. The galaxy has an absolute magnitude range that indicates a small to average size. It exhibits a color gradient, appearing slightly bluer in the central regions and gradually becoming redder towards the outer edges. The object has a low star formation rate. The stellar mass suggests that the galaxy is composed mainly of old, redder stars.
