The galaxy appears to be undergoing a significant interaction or merger event. Multiple distinct luminous cores are visible, suggesting the presence of at least two galaxies in the process of combining. A diffuse, irregular halo of light surrounds these cores, indicative of tidal disruption and gravitational disturbances caused by the interaction. The galaxy does not exhibit a well-defined disk or spiral structure. Instead, the morphology is complex and chaotic, with extended plumes and streamers of material extending away from the central regions. There is evidence of ongoing or recent star formation, particularly concentrated in or near the cores of the interacting galaxies. The overall color of the galaxy appears relatively blue-white, suggesting a population of young, hot stars is present.
