The galaxy exhibits a complex morphology, appearing to be in the late stages of a merger. There is one main bright central body, likely the core of the original galaxy. Just below this is a second prominent bright spot, implying a recent galactic collision. The primary color of the galaxy is yellowish-white, suggesting an older stellar population. A diffuse halo of light surrounds the main structure, possibly indicative of tidal debris resulting from the gravitational interactions. There is evidence of minor disturbances visible in the shape of the galaxy, which are likely caused by gravitational interactions with the other merging galaxy. The system appears relatively smooth overall.