The galaxy presents as a system possibly undergoing or having undergone a merger event. There are two distinct luminosity centers, suggesting two galactic nuclei either in close proximity or currently interacting. The upper nucleus displays a round morphology with a smooth, unresolved texture. This core is bright, exhibiting a high luminosity, with a slightly elongated shape.

The lower nucleus displays a more diffuse and irregular morphology. Patches of slightly bluer light are observed surrounding it, which could be evidence of recent star formation.

There appears to be a faint tidal tail or bridge extending from the main body, which could further support the hypothesis of an interaction or merger. Overall, the system lacks clear spiral arm structure and displays a disrupted morphology, typical of interacting galaxies.
