The galaxy presents a complex morphology, appearing to be in a late stage merger. Two distinct luminous cores are visible, suggesting the presence of two interacting galactic nuclei. These cores exhibit a yellowish-orange hue, potentially indicating an older stellar population and/or significant dust obscuration. The overall shape of the galaxy is highly irregular, with tidal features and distortions suggesting strong gravitational interaction. There is evidence of extended diffuse emission surrounding the primary bodies, indicative of stripped stellar material and gas. A faint, bluish tint is discernible in the outer regions, which may indicate areas of recent or ongoing star formation triggered by the merger event. Dust lanes or patches are not clearly resolved, but the color gradients suggest differential extinction across the system. Overall, the galaxy appears to be a luminous and dynamically disturbed system, likely undergoing a significant transformation as a result of the merger.
