The galaxy presents as a relatively smooth, elliptical structure, elongated in shape. The light is concentrated towards the center, which appears as a bright and somewhat yellow core. There is a smooth, gradual decrease in luminosity moving outward from the core to the outer edges. No distinct spiral arms or dust lanes are apparent. There is a slight orange hue in the extended halo surrounding the core, likely indicative of an older stellar population. There seems to be no signs of a major merger.
