The galaxy appears as a slightly elongated, reddish-orange object, suggesting an elliptical or lenticular morphology. Its light profile is relatively smooth and concentrated towards the center, with a gradual decrease in intensity toward the edges. It is elongated horizontally and has a fairly even brightness distribution. There is no obvious presence of spiral arms or significant dust lanes. Overall the galaxy appears to be relatively undisturbed. The color suggests a population of older stars with relatively little ongoing star formation.
