The galaxy appears to be undergoing a major merger, with a significant interaction and potential tidal features, though these are faint. The morphology is highly disturbed. There are what appear to be two distinct nuclei, suggesting the late stages of the merger. The overall color of the galaxy appears relatively red, possibly indicating an older stellar population or significant dust extinction. There is little evidence of spiral arm structure or a well-defined disk. The galaxy appears relatively smooth in areas, and very concentrated.
