The galaxy presents as a relatively smooth, concentrated object with a slight ellipticity. Its overall color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue at its core, which fades subtly towards a greenish-blue periphery. The color gradient is indicative of a possible decline in recent star formation moving outward from the center, though it's not devoid of it. There's no readily apparent disk structure or distinct spiral arms. The galaxy appears mostly undisturbed, lacking obvious signs of ongoing mergers or major tidal interactions. There is minimal evidence of irregular morphology or significant dust lanes, which supports its classification as an elliptical or lenticular galaxy. 
