The galaxy presents a relatively smooth and concentrated morphology. It is characterized by a central bulge region that exhibits a yellowish hue, indicating a population of older stars. The galaxy appears largely elliptical, with a high degree of central concentration of light. There is subtle indication of possible features or disturbances, but no clearly defined spiral arms or a prominent disk structure are apparent. There is a general gradient in color from the core outwards into the halo that is consistent with a gradual decrease in star formation.
