The galaxy exhibits a disturbed morphology, suggesting a recent or ongoing interaction. A prominent, elongated feature extends from the main galactic body, possibly indicative of tidal forces or a stream of material stripped from the galaxy. Bright knots are visible within the extended feature, which may represent areas of active star formation. The main body of the galaxy appears diffuse and less structured. The overall color suggests a bluer population of stars, which could indicate a period of enhanced star formation. There are several features that suggest a merger is occurring, including disruption of the disk and the tidal tails.