The galaxy appears to be undergoing a significant merger event. The morphology is highly disturbed, displaying prominent tidal features indicative of gravitational interaction. There are two major components, possibly the remnants of the original galaxies. One component is brighter and exhibits a more concentrated structure, while the other is more diffuse and elongated, connected by a faint bridge of material. Patches of intense blue color suggests active star formation in some regions, potentially triggered by the merger. The overall shape is irregular and lacks a well-defined spiral or elliptical structure. The galaxy appears to have a substantial stellar mass and an ongoing high star formation rate.
