The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color profile suggests a population of older stars, indicated by the yellowish-orange hue across the galaxy. There is no evidence of prominent spiral arms or significant dust lanes visible in this image, and the shape is not perfectly round. Minimal, if any, signs of recent major merger events are apparent, with a generally undisturbed morphology.
