The galaxy presents as a single, relatively smooth object. It is spheroidal in shape, exhibiting a high degree of circularity. There is no apparent disk structure or spiral arm morphology visible. The galaxy displays a central concentration of luminosity that fades gradually into the surrounding halo. There are no obvious signs of major mergers or tidal disturbances. The object has a redder hue at the center and becomes bluer with distance from the center. These redder hues suggest an older population of stars at its core. The bluer colors suggests there could be a faint disk. Although, in the outer regions, the galaxy is compact, with no visible extended halo.
