The galaxy presents as a relatively smooth, centrally concentrated object. There is a lack of prominent spiral arm structures or other distinct morphological features. The light distribution appears largely spheroidal, leaning towards a more rounded shape, with a subtle color gradient moving from a bluer outer halo region inward to a more yellow hue at the core. The overall texture indicates a likely smooth distribution of stars. Evidences of minor disturbances can possibly be seen, but there is no indication of major mergers or interactions with other galaxies based on the image.
