The galaxy presents as a single, relatively smooth object with a generally elliptical morphology. There is a central concentration of light. The light emanating from the central region transitions into a dimmer yellowish-white glow. Given the color profile, the galaxy appears to be composed of an older stellar population. There may be a negligible amount of recent star formation occurring. There are no obvious signs of spiral arm structure or a prominent disk. Furthermore, there are no indications of any major ongoing mergers or significant tidal disturbances. The galaxy appears to be largely undisturbed.
