The galaxy presents a somewhat smooth morphology, although there are some features or disks present. It appears to have a generally intermediate roundness, somewhere between round and elongated. The galaxy is likely undergoing a significant merger. The galaxy exhibits a central concentration of light, with a broader, fainter halo extending outwards. The central region appears to be composed of at least two distinct bright knots, possibly galactic nuclei. There is some hint of tidal features or distorted arms, further suggesting an ongoing or recent interaction. There is a central bulge and also some blue light. The galaxy has significant star formation. 