The galaxy appears as a centrally concentrated, relatively smooth object with an overall elliptical morphology. It exhibits a yellowish-orange hue, which suggests a population of older stars. The light profile smoothly decreases from the center outwards with no apparent spiral arms or disk-like structure. There are no obvious signs of recent star formation or significant dust lanes visible in this image. The object has a fairly symmetric shape, but there are some slight irregularities in its outer regions. It appears mostly undisturbed, showing no strong signs of a major merger event. There is a very slight chance of a minor disturbance, but more data is required.
