The galaxy presents a generally smooth, elliptical morphology. The primary body of the galaxy is characterized by a bright, concentrated central region exhibiting a yellowish-orange hue. This suggests a population of older stars. The galaxy shows a gradual decrease in brightness from its core outwards, with no distinct spiral arm structures visible. It has a generally rounded shape with an insignificant elongation. Evidences of major mergers or significant tidal disturbances are absent, suggesting it is a fairly settled system.
