The galaxy presents a complex morphology, appearing to be in a late stage merger event. Two distinct, bright nuclei are visible, exhibiting a yellowish hue, suggestive of an older stellar population or significant dust obscuration. Tidal features are evident, with diffuse streams of material extending outward from the main bodies, indicating gravitational interaction and disruption. A faint, elongated structure connects the two nuclei, possibly a bridge of gas and stars formed during the merging process. The overall color is relatively red, implying a low rate of ongoing star formation. The shape is highly irregular, deviating significantly from a typical spiral or elliptical morphology due to the ongoing interaction. The system exhibits signs of significant disturbance, indicative of a dynamic and evolving system.
