The galaxy presents as a relatively smooth, elliptical structure. Its color profile suggests a dominant population of older stars, with a notable lack of blue hues indicative of recent or ongoing star formation. The galaxy's shape is close to circular, exhibiting minimal elongation or asymmetry. There is no visually apparent evidence of spiral arms or a distinct disk component. The overall appearance indicates a galaxy that is dynamically relaxed and evolved, consistent with a classification as an early-type galaxy. The light distribution is concentrated toward the center.
