The galaxy presents a generally smooth and rounded morphology. It appears elliptical in shape, with a noticeable central bulge that exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy diffuse outwards, showing a bluer color, which could indicate the presence of younger stars. There's no evidence of strong spiral arm structures or major disturbances indicative of recent mergers, though a slight asymmetry cannot be ruled out. Overall, the galaxy seems relatively isolated and quiescent.
