The galaxy appears to be undergoing a merger or interaction. It exhibits a relatively smooth overall morphology. There is a primary, more elongated component that has a reddish-orange hue. Juxtaposed to this is a bluer, more circular component. Given the color difference, there appears to be a contrast in the stellar populations within each component, with the redder galaxy exhibiting a potentially older stellar population and the bluer one being actively forming stars. There is a slight indication of tidal features or disturbances, but the overall structure remains fairly cohesive. The galaxy is not perfectly round; it is more elongated.
