The galaxy appears as a centrally concentrated, ellipsoidal object. Its core is a bright, diffuse, and almost unresolved region that seems to blend smoothly with the surrounding halo. The galaxy's color gradient transitions gradually from a slightly bluer hue in the outer regions to a more uniform distribution throughout. There are no apparent spiral arm structures, and the disk component is either absent or oriented face-on relative to the observer. The overall morphology indicates an evolved stellar population, suggesting minimal recent star formation. It exhibits a smooth, non-disturbed structure, with no signs of active galactic nuclei or major tidal disturbances. It appears to be isolated, with no nearby interacting companions visible in this field of view.
