The galaxy presents a roughly elliptical morphology. It appears as a diffuse object with a slightly elongated shape, its major axis being a few times longer than its minor axis. The overall color profile suggests a relatively old stellar population, though there are hints of bluer regions implying some ongoing star formation. A small fraction of the galaxy seems disturbed, possibly indicating that it may have gone through a minor merger in its past. A significant component of the galaxy is composed of a smooth distribution of stars, though the outer regions appear slightly less uniform. The central part seems very round in comparison to the edges. 
