The galaxy appears to be undergoing a major merger event. Two distinct galactic nuclei are visible, indicating the presence of two progenitor galaxies in the process of coalescence. These nuclei are connected by a bridge of luminous material, suggesting tidal interactions and ongoing gravitational disturbances. The overall morphology is highly disturbed and asymmetric, lacking a well-defined spiral or elliptical structure. Evidence of significant star formation may be present, inferred from the bluish-white colors of the galactic nuclei. The galaxy exhibits a diffuse halo and a complex network of tidal tails and debris, resulting from the violent merging process. A significant amount of dust is possibly present, causing extinction, and reddening of the galactic light at certain locations.
