The galaxy presents as a relatively smooth, elongated structure. It appears to be an elliptical galaxy viewed at an oblique angle. There is a color gradient within the galaxy, the central region displaying a more yellow hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, which could be indicative of some ongoing, albeit subdued, star formation. There are no spiral arms or prominent dust lanes visible. The overall morphology suggests a significant fraction of stars with random orbits. It displays a small size as it is fairly far away.
