The galaxy appears to be undergoing a major merging event, with two distinct, bright nuclei visible. The overall morphology is highly disturbed, showing little evidence of a well-defined disk or spiral structure. The dominant color is yellowish-orange. There is a slight blue tint to the merging area, indicating the presence of at least some younger, hotter stars, likely formed as a result of the ongoing merger. The galaxy is relatively compact in apparent size.
