The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology with a high degree of roundness. There is a prominent central bulge that appears to be the brightest region of the galaxy. The outer regions show a gradual decrease in luminosity, indicating a smooth transition from the core to the halo. There is no clear evidence of spiral arm structures or significant dust lanes. Faint color variations are present, with a hint of bluer hues in the inner regions and redder colors in the outer regions. The overall structure suggests minimal signs of recent mergers or major disturbances.
