The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is elliptical to slightly rounded. The color profile suggests a higher concentration of older stars, particularly in the central region. The core of the galaxy exhibits a bright, yellowish-white hue, possibly indicative of a significant population of evolved stars or a low level active galactic nucleus. Faint, diffuse outer regions extend from the core, displaying a bluer color that may imply some degree of ongoing, albeit limited, star formation within the galaxy's outskirts. There are no discernable spiral arms or prominent dust lanes, further supporting its classification as an elliptical galaxy. Based on the observed morphology, the galaxy appears to be in a relatively quiescent state, lacking evidence of major mergers or significant tidal disturbances.
