The galaxy presents as a single, concentrated luminous body with a smooth, elliptical morphology. The color gradient suggests an older stellar population, with the core exhibiting a yellow-orange hue indicative of evolved stars. The outer regions appear slightly bluer, potentially indicating pockets of more recent, albeit minimal, star formation activity. There is no visual evidence of a prominent disk structure, spiral arms, or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. The overall structure suggests a well-evolved galaxy, likely residing in a relatively dense environment, and undergoing low levels of star formation.
