The galaxy presents a somewhat irregular morphology, exhibiting a clumpy and disturbed structure, likely in the early stages of a major merger event. The light profile appears concentrated in two distinct regions, indicating multiple galactic nuclei possibly undergoing coalescence. The dominant color is a notable blue hue, suggestive of ongoing or recent star formation activity within at least one of the merging components. There are no obvious spiral arms or a well-defined disk. Overall, this galaxy seems to be experiencing significant gravitational interactions, leading to a non-equilibrium configuration.
