The galaxy appears to be undergoing a significant merger event. The system displays a dual-core structure, with two distinct concentrations of light visible, suggesting the presence of two galactic nuclei. A diffuse, irregular halo of light surrounds the central region, indicating tidal interactions and disruption of the original galactic structures. The overall color gradient transitions from bluer hues in the lower section to redder hues in the upper section. A higher proportion of the light appears to be centered toward the redder section of the galaxy. The morphology is disturbed, showing no clear spiral arms or elliptical structure, consistent with late-stage merging activity. There is a possible dust lane that bisects the galaxy. Overall, the system appears to be in a highly dynamic state, with ongoing gravitational interactions likely triggering bursts of star formation.
