This galaxy appears to be undergoing a significant merger event. The primary body exhibits a somewhat amorphous structure with a flattened, disk-like component. The morphology suggests the possibility of a spiral galaxy, but strong tidal features obscure a definitive classification. A luminous central region is visible, surrounded by a more diffuse halo of light. There is also a very bright region, suggestive of intense star formation, that appears separate from the main structure of the galaxy. The galaxy exhibits disturbed morphology, particularly in the form of extended tidal tails or plumes. The overall color profile suggests a mix of stellar populations, with some bluer regions that likely indicate recent star formation and redder regions which suggest older stellar populations. The galaxy's orientation is approximately edge-on or highly inclined, making it difficult to fully discern its internal structure.
