The galaxy appears to be undergoing a significant interaction, possibly a merger, with another galactic body. The primary component exhibits a generally smooth morphology, with a roughly elliptical shape. There are hints of tidal features or disturbed structures in the outer regions, suggesting gravitational interaction. The core region displays a high concentration of older stars, indicated by the yellowish-orange hue. A smaller, distinct component lies nearby, appearing more compact and also yellowish-orange. There is an overall reddish color, indicating a population of older stars and relatively low star formation activity.
