The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a relatively even brightness distribution, suggesting an older stellar population. The galaxy's overall color appears redder, indicative of a population of older, cooler stars and potentially a low rate of ongoing star formation. There is a very faint disk-like structure. No spiral arms are visible. The galaxy seems relatively undisturbed, showing no signs of major mergers or tidal interactions, although a minor disturbance cannot be ruled out.
