This galaxy appears to be undergoing a significant merger event. Two distinct galactic nuclei are visible, one displaying a yellowish hue and the other presenting a bluer color. There is evidence of tidal disruption between the two components, suggesting a strong gravitational interaction. The overall shape deviates significantly from a smooth elliptical or spiral form; the morphology is irregular, with complex structures and disturbances. There appears to be extended, diffuse emission surrounding the main bodies, likely composed of stars stripped from the merging galaxies. Within the primary components, there is a notable color gradient, suggesting varying stellar populations or dust extinction effects. Overall, the galaxy is categorized by its active merger state and disturbed morphology.
