The galaxy presents a morphology indicative of a system undergoing a major merger. There are two distinct, luminous components, potentially representing the remnant cores of the progenitor galaxies. These cores exhibit a somewhat rounded shape. There is evidence of tidal distortion, as the galaxy does not possess a clear, regular structure. Diffuse light extends between and around the cores. The overall color is yellowish, suggesting an older stellar population with lower rates of current star formation.
