The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, with a high degree of circularity. There is a suggestion of a faint, extended halo surrounding the central region, but the image lacks the resolution to determine distinct structures such as spiral arms or a prominent disk. The galaxy exhibits a color gradient, appearing bluer towards the center and redder in the outer regions, which may suggest different stellar populations or dust distribution. There are no obvious signs of tidal disturbances or ongoing mergers, and appears to be relatively undisturbed. The light distribution of the galaxy smoothly decreases away from the core, indicating a lack of any strong star forming regions.
