The galaxy presents a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue, indicative of an older stellar population. The galaxy lacks prominent spiral arm structures or significant dust lanes. There is a slight elongation in its shape, deviating minimally from a perfect circle. Some subtle disturbances may be present within the outer regions of the galaxy, but they are faint. Overall, the galaxy appears relatively undisturbed, not exhibiting any signs of ongoing major mergers.
