The galaxy presents as a centrally concentrated object with a smooth light distribution. The core region exhibits a bright, yellow-orange hue, which fades into a blue-green outer region. The galaxy appears roughly elliptical in shape, showing no strong evidence of spiral arms or a distinct disk structure. There is also no readily apparent signs of a major merger. It exhibits a relatively smooth, rounded structure with no distinct features or significant disturbances visible. The overall morphology suggests a system dominated by an older stellar population and a low rate of star formation.
