The galaxy presents as a relatively smooth, centrally concentrated object, appearing elliptical in shape. The core region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The light gradually fades towards the outer regions, which appear more diffuse and less distinctly colored, indicating a decreasing density of stars. There are no obvious spiral arm structures or significant dust lanes visible. Minor irregularities hint at possible gravitational disturbances, but overall it exhibits a settled morphology.
