The object appears to be a relatively smooth, elliptical galaxy. Its light profile suggests a central concentration of stars, perhaps indicating an older stellar population. There's a noticeable color gradient, with a yellower, brighter core that fades into a bluer halo, suggesting different stellar populations or dust distribution within the galaxy. The overall morphology does not show any distinct spiral arms or significant disturbances, potentially indicating a lack of recent major mergers. A slight elongation is observed, but it's close to being a circular shape.
