This galaxy appears to be in the late stages of a merger. There are two distinct, bright nuclei visible. The light distribution from each nucleus is fairly smooth. Around each nucleus, there appears to be a diffuse stellar halo. The overall shape is somewhat irregular, suggesting gravitational disturbance, but there are no tidal tails visible. There may be minimal ongoing star formation, as indicated by the slight greenish tint, but the dominant color is reddish-yellow, indicating an older stellar population. The galaxy is relatively compact. It presents as moderately round, with a slight tendency toward a more elliptical shape.
