The galaxy appears to be a relatively faint, blue-tinged object with a disturbed morphology. A central, brighter region is visible, suggesting a concentration of older stars or an active galactic nucleus, though the resolution is insufficient to confirm the presence of the latter. There are asymmetrical, diffuse extensions or tidal tails. The overall structure appears to be undergoing a significant interaction or possible ongoing merger. The blue color suggests the presence of younger stars, although this might be because of decreased dust extinction in those areas. Evidence for substantial ongoing star formation is not clearly discernible from visual inspection alone but based on the color gradients it does not seem quiescent.
