The galaxy presents an elliptical morphology, appearing mostly smooth and well-resolved. Its colour profile indicates a dominant population of older stars, as evidenced by the yellowish-red hue. There seems to be evidence of interaction or a recent merger, characterized by a disturbed morphology. There is a bright, relatively compact core, which fades towards the outer edges of the galaxy. There appears to be a faint second core next to it, supporting that this could be a recent merger. The overall shape is fairly rounded.
