The galaxy presents as a fairly symmetrical, elliptical morphology, with a smooth, concentrated light profile. Its core is a bright, yellowish-orange hue, suggesting a population of older stars. There's a gradual decrease in surface brightness moving outward from the core, with the outer regions displaying a redder color, possibly indicating the presence of dust or a population of cooler, redder stars. There's a notable absence of spiral arms or distinct features typically associated with actively star-forming galaxies. Based on its color and morphology, it appears to be a relatively massive galaxy that is no longer actively forming stars. 
