The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The color profile suggests a relatively old stellar population, with a dominant yellowish-orange hue in the core region. There is a faint, diffuse halo surrounding the central bulge, transitioning into a dimmer, less defined outer region. The galaxy appears relatively isolated with no obvious signs of ongoing major mergers or significant tidal disturbances. There are slight color variations throughout the galaxy. The center is more yellow than the green-blue edges.
