The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its light is dominated by a yellowish-orange hue, indicating a population of older stars. There is minimal evidence of spiral arms or significant dust lanes. The galaxy exhibits a high degree of roundness, suggesting a classification towards an E type galaxy. There is no obvious presence of a strong, actively star-forming nucleus, nor any visible signs of on-going mergers or major disturbances in its structure.
