The galaxy presents a complex morphology indicative of an ongoing or recent interaction. A dominant, relatively smooth and bright central component is observed. This component exhibits a somewhat round appearance, although deviations from perfect circularity are apparent. To one side, a fainter, more diffuse extension is observed, possibly representing a tidal feature or disrupted galactic arm. The color gradient across the galaxy suggests varying stellar populations, with the central region appearing bluer compared to the slightly redder outer regions and extensions. Overall, the system is not clearly defined, showing signs of gravitational disturbance.
