The galaxy appears to be a relatively smooth, elliptical system, exhibiting a generally spheroidal morphology. The core is a bright, concentrated region showing a yellow-orange hue, indicating an older stellar population.  The galaxy fades gradually outward, with the outer regions appearing less defined and possessing a bluer tint. There is no apparent disk structure or spiral arm features.  Indications of mergers or major disturbances are not immediately obvious, although some minor irregularities in the outer regions cannot be ruled out. Overall, the galaxy's profile suggests it is a well-evolved, relatively quiescent system.
