The galaxy appears to be undergoing a significant merger event, with several distinct nuclei visible. The primary component exhibits a somewhat amorphous, rounded morphology, though tidal features or distortions suggest gravitational interaction. Two less prominent, but still clearly defined nuclei are observed in close proximity to the main body, perhaps representing the cores of merging galaxies. There appears to be an additional clump of red light above the center of the galaxy, which could be another merging element, an area of intense star formation, or an artifact. The overall color is yellowish-orange, indicative of an older stellar population or significant dust obscuration. Evidence of a disk structure is minimal, which might be due to the ongoing merger disrupting any pre-existing order, or because the intrinsic structure of the galaxies involved are elliptical or irregular in nature.
