This galaxy exhibits a morphology indicative of a system undergoing a significant merger event. There appear to be two distinct, luminous concentrations, likely representing the cores of the progenitor galaxies. These cores are embedded within a fainter, diffuse halo of stellar material. The light distribution is smooth and concentrated toward the center, suggesting an advanced stage of merging where the individual galactic structures are beginning to coalesce. There is evidence of tidal features or disturbed morphology in the outskirts, consistent with gravitational interactions. Overall, this system suggests a galaxy in transition towards a more relaxed, elliptical-like morphology as a consequence of the ongoing merger.
