The galaxy presents a morphology indicative of a merging system. Two distinct components are discernible. One component exhibits a smoother, more diffuse light distribution, potentially indicating an elliptical or spheroidal galaxy. The other component seems to display a disk-like structure with signs of tidal disruption. The disk appears to be undergoing significant disturbance and deformation, likely due to gravitational interactions with its companion. The overall color suggests ongoing star formation, particularly in the disrupted disk component, with possibly a more quiescent stellar population in the smoother elliptical component. The system appears to be in an advanced stage of merging based on the strong distortions observed.
