The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the structure, appearing a warm yellowish-orange hue. The outer regions of the galaxy exhibit a fainter, bluish-greenish glow, suggesting the presence of a younger stellar population compared to the core. There is a slight elongation noticeable, giving the galaxy a somewhat oblate shape. No prominent spiral arms or significant dust lanes are readily apparent in the image. Faint asymmetries or minor disturbances can be seen upon closer inspection of the light distribution in the outer disk, although there's no clear evidence of ongoing major merger activity. Overall, the system seems to be a relatively undisturbed and evolved galaxy.