The galaxy exhibits a morphology that appears to be undergoing a significant merger event. The primary structure of the galaxy shows evidence of two distinct, bright nuclei or central concentrations of stellar mass, suggesting a recent or ongoing collision of two galaxies. These bright regions are somewhat rounded, which can be consistent with galaxies which have not yet fully distorted each other.

The overall color profile appears to be on the redder side, indicating a population of older stars, or significant dust obscuration. Star formation appears suppressed or slowed down, which might be caused by tidal forces experienced due to the ongoing merging process. There is a lack of well-defined spiral arm structures or a distinct disk shape.
