The galaxy presents as a relatively smooth, elliptical morphology. There is a high degree of central concentration, with a gradual decrease in luminosity towards the outer edges. The galaxy exhibits a yellow hue, suggesting a population of older stars. There is no apparent spiral structure or dust lanes visible. The overall appearance indicates a galaxy that is likely spheroidal in shape, with minimal signs of recent star formation. The smoothness of the light distribution suggests that it is a relatively undisturbed system, with no signs of major mergers or tidal interactions. The lack of bluer colors or irregular features implies a well-evolved stellar population and an absence of ongoing star formation.
