The galaxy appears to be undergoing a significant merger event. Two distinct galactic nuclei are visible, with the larger of the two displaying a more pronounced central bulge. The overall shape is irregular, deviating significantly from a standard elliptical or spiral morphology. There is some diffuse emission surrounding the main bodies, hinting at tidal interactions and ongoing star formation triggered by the merger. The light distribution indicates a potential redder color, possibly due to a higher proportion of older stars and dust obscuration, which could be expected in a merging system. The two nuclei are close in proximity, suggesting we are observing the merger in a fairly late stage. Faint extensions can possibly be seen in a couple of the directions away from the central body.
