The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical or lenticular, with a generally elongated shape. There's a noticeable color gradient across the galaxy. The central region exhibits a yellow-orange hue, suggesting a population of older stars, while the outer regions show a bluer tint, hinting at younger stellar populations or potential star formation. Overall, this galaxy seems to be relatively evolved and likely possesses a substantial stellar mass. Star formation appears to be occurring at a low rate. No signs of significant ongoing mergers are apparent.
