The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. There appears to be two primary concentrations of light, possibly representing the cores of the merging galaxies. These cores are approximately equidistant from each other. A diffuse, extended halo of fainter light surrounds the galaxy, likely composed of tidal debris resulting from gravitational interactions. The central region displays a yellowish-white hue, potentially indicating an older stellar population or significant dust obscuration. There are hints of bluer regions within the outer parts of the galaxy, indicative of more recent star formation, possibly triggered by the merger. The overall shape is neither purely elliptical nor spiral, reflecting the irregular nature of the merging system. Based on these observations, the galaxy is estimated to be a relatively massive system with a moderate rate of star formation.
