The galaxy presents as a complex system, seemingly undergoing a merger event. Two distinct, bright, yellowish-orange cores are visible. One core is brighter and slightly larger than the other. These may be the original nuclei of the merging galaxies.

A fainter, bluer tidal tail or stream extends away from the cores, indicating ongoing gravitational interactions. This blue coloration suggests recent or current star formation within the tail, likely triggered by the merger.

The overall shape of the system is disturbed, lacking a clear, defined structure. This is consistent with the ongoing merging process, which is disrupting the original morphologies of the progenitor galaxies. The relative brightness in g, r, and z bands suggest a luminosity typical of larger galaxies. The relatively high Sersic index suggests an elliptical component, which is consistent with the galaxy being the result of a merger event.
