This galaxy exhibits a complex morphology, appearing to be in a state of interaction or merging. The primary galactic body shows a somewhat distorted disk-like structure with apparent tidal features. The central region is bright, potentially indicating an active galactic nucleus or a high concentration of stars. The disk is not uniform and seems to display clumps and asymmetries.

A secondary structure, possibly another galaxy, shows a more uniform, smooth morphology, and is positioned seemingly very close to the primary galaxy. This could indicate a merger or tidal interaction. There appears to be a faint bridge of material extending from the lower end of the primary galaxy towards this smooth structure.
