The object presents as a merging system of two distinct galactic nuclei. The larger nucleus exhibits a smoother profile, appearing nearly spherical, with a concentrated bright core and a more diffuse halo. Its color is shifted to the redder part of the spectrum. The smaller nucleus, positioned slightly offset from the larger one, displays a more yellowish, less extended profile. There are no readily apparent spiral arm structures or strong dust lane features visible in either nucleus. Tidal features or faint extensions are subtly visible and suggest ongoing gravitational interaction between the two galaxies. Overall, the merging system appears to be in a relatively advanced stage of interaction.
