The galaxy presents a generally smooth and elliptical morphology. There is a prominent central bulge with a high degree of concentration. The color profile suggests a relatively old stellar population, with a yellowish-orange hue dominating the core region, possibly indicating the presence of evolved red giant stars. There are faint signs of what appears to be a disk with no clear spiral arm structure visible. The overall structure is relatively undisturbed, with no major signs of ongoing merger activity.
