The galaxy presents a flattened, disk-like morphology viewed at an oblique angle. The central region exhibits a bright, concentrated luminosity, potentially indicating a dense stellar population or active galactic nucleus. Surrounding this central region is a ring-like structure of enhanced emission. Within this ring, some knotty or clumpy structures are visible, possibly representing regions of active star formation. There is a hint of a spiral arm structure within the clumpy ring, but it is faint and difficult to fully characterize. The overall color of the galaxy appears shifted towards the green. No obvious signs of recent major merger events or significant tidal disturbances are apparent, although there could be minor disturbances affecting the overall shape of the galaxy. The overall distribution of light is smooth and concentrated.
