The galaxy presents a flattened elliptical morphology. The central region exhibits a high surface brightness, appearing as a concentrated bulge. The galaxy's light profile demonstrates a smooth gradient outwards from the core, indicative of an evolved stellar population. There is little indication of spiral arm structure or prominent dust lanes, leading to an classification as early type. The color index suggests a relatively red population of stars consistent with a lack of significant ongoing star formation. Small disturbances are present in the halo. Overall the galaxy is not perfectly round and is slightly oblong.
