The galaxy presents a flattened, elliptical morphology, appearing somewhat disk-like when viewed from our vantage point. It exhibits a central, slightly brighter bulge. The overall color is predominantly bluish-white, suggesting a population of relatively young, hot stars. Some faint dust lanes are potentially visible upon close inspection, indicating the presence of interstellar matter. There appear to be some disturbances as the light of the galaxy is scattered around the central bulge, which might suggest a merger or disturbance event. There is no spiral structure easily visible, and it appears mostly smooth in nature. The galaxy is relatively compact in size, and it displays a concentrated central region.
