The galaxy appears to be undergoing a significant merger event. There are clear signs of tidal disruption, with a disturbed morphology. One of the merging components shows a reddish-yellow hue, potentially indicating an older stellar population or significant dust obscuration, while the other exhibits a bluer color. The overall shape is elongated and irregular, deviating significantly from a typical elliptical or spiral structure. There is a distinct tail-like feature extending from one side, suggestive of gravitational interaction and material stripped during the merger. No defined spiral arms or a central bulge are clearly visible in the overall merging system.
