The galaxy appears as a single, relatively smooth object. Its morphology is largely spheroidal, exhibiting a high degree of circular symmetry. The light distribution suggests a centrally concentrated structure, with brightness decreasing smoothly from the core outwards. There is no apparent spiral arm structure or distinct disk component visible within the limits of the image resolution. The color of the galaxy is slightly redder than the average color of the sky around it, with some yellow-ish tint. It may be consistent with an elliptical galaxy consisting primarily of older stellar populations. The presence of a possible minor gravitational disturbance cannot be ruled out completely, but no major interaction or merger event is evident in this image.
