The galaxy presents as a moderately luminous system with an elongated, cigar-like morphology. The primary structure appears to be relatively smooth, though some irregular features are suggested by the light distribution, which exhibits possible minor disturbances. A faint blue region is visible, potentially indicative of younger stars or active star formation. A reddish component is also visible, potentially indicating older stars and dust absorption. Overall, the galaxy shows hints of potential interactions or recent mergers, based on its irregular structure and elongated shape.
