The galaxy presents as a centrally concentrated object, roughly circular in projection. It exhibits a smooth, featureless morphology, lacking discernible spiral arms or a distinct galactic disk. The core region displays a yellowish hue, suggesting an older stellar population and/or dust obscuration. The outer regions of the galaxy appear fainter, with a gradual decrease in luminosity towards the edges. There are no obvious signs of ongoing mergers, tidal tails, or other significant disturbances in its overall structure.
