The galaxy presents as a generally smooth, elliptical structure with a moderate degree of elongation. The central region is characterized by a high concentration of light, appearing as a bright, yellowish core. This suggests a significant population of older stars. Moving outwards from the core, the galaxy exhibits a gradual decrease in surface brightness. Faint blue hues are visible in the outer regions, potentially indicative of a younger stellar population and ongoing, albeit low-level, star formation. There are no obvious spiral arm structures or strong dust lanes visible in this image, and only minor disturbances to it's structure which suggests no recent major merger events.
