The galaxy appears as a relatively smooth, centrally concentrated object. It presents a nearly circular morphology with a gradual decrease in luminosity from the core outwards. The color profile suggests an evolved stellar population, exhibiting a yellowish hue throughout the majority of its structure. There is no apparent spiral structure, bar, or significant dust lane obscuration visible in this image. The overall appearance is consistent with that of an elliptical galaxy, with no signs of recent major merger activity or significant tidal disturbances. The light is concentrated in the central region.
