The galaxy presents a complex morphology, appearing to be in the late stages of a major merger. Two distinct nuclei are visible, suggesting the collision of two significant progenitor galaxies. The upper nucleus exhibits a reddish hue, potentially indicating an older stellar population or significant dust obscuration. The lower nucleus displays a yellowish-white color, suggesting a mix of stellar ages. A faint tidal tail or bridge of material extends outwards, indicative of gravitational interaction. The overall structure is disturbed, lacking the smooth, symmetrical form of a relaxed elliptical galaxy or well-defined spiral arms of a spiral galaxy. There is evidence of active or recent star formation within the system. The light from the galaxy appears to be moderately redshifted.
