The galaxy presents as a somewhat elongated elliptical or lenticular system. It exhibits a smooth, centrally concentrated light distribution, with a relatively featureless overall appearance. The core region displays a yellowish hue, which might suggest a population of older stars. Moving outward from the core, the color shifts subtly towards bluer shades. This could indicate the presence of some younger stellar populations in the galaxy's outer regions, or possibly some ongoing, but limited, star formation. There is no apparent spiral arm structure, nor are there any major disturbances or signs of ongoing mergers visible in the image, although there may be minor disturbances present. The galaxy appears relatively isolated and undisturbed.
