The galaxy presents as a system undergoing a significant merger event. Two distinct nuclei are visible, suggesting two progenitor galaxies are in the process of coalescing. The system exhibits a disturbed morphology, lacking a well-defined spiral or elliptical structure. There is a prominent tidal tail or bridge of stellar material extending from the primary body of the galaxy, indicating gravitational interaction and disruption. The color appears bluer in the central regions, which potentially indicates ongoing star formation, while the outer regions appear redder. It appears to be a relatively small galaxy.
