The galaxy appears to be undergoing a significant interaction or merger with another galaxy. There is a double nucleus visible, which is fairly common in merging galaxies. The galaxy on the right has a strong smooth profile, whereas the galaxy on the left is slightly more diffuse. The overall morphology is disturbed, exhibiting characteristics suggesting late-stage merger activity. There are no distinct spiral arms or a clear disk structure visible. The primary light from the nuclei seem to have a somewhat redder color profile. There is a faint bluer tinge in the galaxy on the left.
