The galaxy presents as a merging system, exhibiting a disturbed morphology. Evident are two distinct nuclei, indicating the interaction of two separate galactic bodies. The overall color profile suggests a mix of stellar populations, with some regions appearing more yellow/red, implying older or dustier regions, while others show bluer hues, possibly indicative of more recent star formation. The tidal features suggest significant gravitational interaction and disturbance, potentially leading to eventual galactic merging. The galaxy's shape deviates significantly from a smooth elliptical or spiral structure, displaying irregular features consistent with ongoing mergers.
