This galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger event. The primary component presents a relatively smooth, rounded profile, with a concentration of light suggesting an older stellar population. Adjacent to this, another distinct concentration of light shows evidence of active star formation, indicated by a more prominent blue-green hue. The overall system displays signs of tidal disruption, with diffuse, extended features suggesting the presence of tidal tails or bridges. The irregular shape and disturbed morphology indicate a system that is far from equilibrium, likely resulting from the gravitational interaction with another galaxy. There may also be a small object to the right of the galaxy appearing more red-shifted than the primary galaxy. 
