The galaxy exhibits a morphology suggesting an ongoing or recent interaction or merger. It appears to be composed of two distinct components. The primary component is a centrally concentrated, relatively smooth region that appears somewhat elliptical. A secondary, smaller, and bluer component is observed adjacent to the primary. The overall color of the system is somewhat blue-white, suggestive of ongoing star formation. There is a notable disturbance to the morphology, potentially tidal features or irregular arms, indicative of a disruption.
