The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that graduates outwards into a more diffuse halo. Color gradients are subtle, but an overall yellowish hue is apparent, indicating a possible older stellar population. There's little evidence of prominent spiral arms or active star formation regions, and its apparent spheroidal shape suggests it is an elliptical galaxy that is very round. The galaxy appears to be relatively isolated, lacking any signs of major tidal disturbances or ongoing mergers, although some minor disturbance cannot be ruled out. The edges are quite faded into the black background.