The galaxy presents as a single, relatively smooth and concentrated object. There is no apparent spiral structure, bar, or disk visible. The light appears to be fairly uniform across the body of the galaxy. There is a subtle color gradient visible, shifting from slightly bluer towards the center to redder hues at the edges of the visible light distribution. This could be indicative of older stellar populations being dominant in the outer regions of the galaxy. There appears to be a very minor asymmetry or perturbation on one side, which is possibly indicative of a minor interaction. The galaxy appears to be roughly circular, possibly slightly elliptical.
