The galaxy appears as a single, relatively smooth concentration of light. It displays a primarily elliptical morphology, with no distinct spiral arms or a prominent central bar visible. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the outer regions. The galaxy presents an orange hue suggesting a population of older stars, and appears mostly devoid of dust lanes or regions of active star formation. The overall structure suggests a galaxy that has undergone significant evolution, possibly representing a passively evolving system.
