The galaxy displays a complex morphology, potentially indicative of an ongoing or recent interaction. A dominant, relatively bright, and diffuse component with a yellowish hue is observed, possibly an elliptical galaxy. Located near this galaxy is a second, smaller blueish component. It appears elongated and disk-like. A third component with a reddish color is observed, but this could be another galaxy or part of the main galaxy. The system exhibits possible signs of tidal disturbances. The presence of the multiple components suggest a merger. Star formation appears to be active in this region, concentrated in some areas more than others.
