The galaxy presents as a primarily smooth, elliptical structure. The central bulge appears concentrated and exhibits a yellowish hue, suggesting a population of older, evolved stars. The outer regions of the galaxy display a gradual decrease in surface brightness, fading into the background sky. While the overall morphology is smooth, there are subtle indications of a possible faint disk component, most likely composed of older stars. There are no prominent spiral arms or distinct dust lanes visible. There is no obvious sign of interaction or recent major merging activity. It is neither perfectly round nor highly elongated in shape; more an "in-between" ellipticity. Overall, the galaxy seems relatively undisturbed.
