This galaxy exhibits a complex morphology suggestive of a recent or ongoing interaction. The primary body of the galaxy appears diffuse and elongated. A notable feature is the prominent tidal tail extending from the main body, indicating gravitational disruption. There also seems to be a faint bridge-like structure extending to the upper left of the galaxy. The overall color is generally blue-white indicating the presence of hot, young stars, which may have formed as a result of the interaction. The galaxy displays an irregular shape, lacking a clear disk or spiral arm structure. Its morphology is dominated by irregular, clumpy features, some which are denser and brighter, suggesting regions of enhanced star formation.
