The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is somewhat elliptical, not perfectly spherical, leaning towards an in-between elliptical. The central region exhibits a bright, yellowish-white hue, suggesting an older stellar population. The outer regions display a gradual decrease in brightness, transitioning towards a more diffuse, reddish color. There is no discernible evidence of spiral arm structure or a prominent disk. Faint hints of minor disturbances may be present in its overall shape, but no major mergers are apparent.
