The galaxy presents an apparent disturbed morphology, suggesting a possible ongoing merger event. The primary body of the galaxy exhibits a diffuse, slightly elongated structure. There is a secondary, brighter nucleus-like structure situated close to the main body, appearing as a distinct component involved in a possible interaction. The color profile suggests a mix of stellar populations; the central region appears yellowish, hinting at older stars, while bluer tints are observed in the less defined outer regions, suggesting ongoing star formation. The overall light distribution is centrally concentrated. The galaxy appears to be actively undergoing structural changes.
