The galaxy presents as a luminous central bulge that dominates the overall structure. The color of the bulge appears to be yellowish-orange, possibly indicating an older stellar population. Fainter and slightly bluer light is distributed within the bulge as well as a very faint disk structure. There appears to be minimal discernible spiral arm structure or significant dust lanes in the images, suggesting a relatively smooth morphology. The galaxy's shape is somewhere between round and elliptical. There are no obvious signs of major ongoing mergers or strong tidal interactions in the image, although some minor disturbances may be present. This could indicate past interactions or internal processes affecting the galactic structure.
