The galaxy exhibits a complex morphology, suggesting an ongoing or recent interaction. There are two distinct bright cores present, with asymmetric distributions of light suggesting a potential late stage merger. These cores display a yellowish hue. The overall shape can be described as intermediate between round and elongated. Some faint wispy structures are noticeable, potentially tidal tails resulting from gravitational interactions. The outer regions display a bluer tint, suggestive of more recent star formation within those regions. The system overall appears to be actively evolving, exhibiting characteristics of a dynamic system.
