The galaxy presents a complex morphology, seemingly undergoing a significant interaction or merger. Its overall structure is highly irregular and asymmetric, with an elongated shape approximately 10 kiloparsecs across. There is a dominant orange core with what looks like a smaller bright knot at the bottom. A plume-like feature extends away from the central region and is visible toward the top end. The overall color profile leans toward the redder end of the spectrum, possibly indicating an older stellar population or significant dust obscuration. There is some evidence of disturbances, which lends credence to the interpretation that it is an interacting or merging system.
