The galaxy appears to be undergoing a merger or interaction. There are at least two distinct nuclei visible, with a diffuse, extended halo of light surrounding them. The overall color profile indicates a relatively old stellar population, with a significant amount of red light emitted. This is interspersed with blue light from more recent star formation.

One of the nuclei is more centrally located within the galaxy's main body and is brighter than the other. The secondary nucleus is less defined and seems to be located at the end of a long tidal tail extending outward. The tidal tail exhibits a smoother texture, implying that it's undergoing more gravitational stripping of its stars. Overall, the galaxy is smooth in appearance, indicating a high level of internal organization. 