The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light distribution, with a gradual decrease in surface brightness towards the outer regions. There is a slightly redder hue toward the central region of the galaxy and a slightly bluer halo. The galaxy appears fairly isolated and undisturbed, showing no obvious signs of tidal interactions or ongoing mergers. It is generally round in shape and does not appear to be heavily dust-obscured.