The galaxy presents as a single, relatively smooth, and concentrated object. It exhibits a yellowish-white color gradient towards the center, suggesting a higher density of older stellar populations in the core. The overall morphology appears elliptical or spheroidal, with a high degree of circularity. There is no obvious spiral arm structure or prominent disk features visible in this image. Minor disturbances may be present, but they are not obvious, and the galaxy does not appear to be undergoing a major merger, though there is a very slight chance it could be undergoing a minor disturbance.
