The galaxy presents as a generally smooth, elliptical form. Its overall color appears to be a warm, yellowish-orange, suggesting an older stellar population, though some blue-green light is present in the outer regions, possibly indicating the presence of some younger, hotter stars. The galaxy appears somewhat elongated. There is no readily apparent spiral structure or evidence of a prominent galactic bulge. There appears to be some minor disturbance in the system possibly due to a past merger. The galaxy's light is relatively concentrated toward the center, with a gradual decrease in intensity towards the outer edges.
