The galaxy appears to be an elliptical galaxy. The galaxy exhibits a smooth, concentrated light profile, with the highest intensity light concentrated in the galaxy's core and gradually fading outwards into the halo. The galaxy is fairly round. There are no obvious signs of spiral arms or a disk structure, nor any obvious indications of recent or ongoing major mergers or tidal disturbances in the image. There may be minor disturbances due to the clumpy shape of the low intensity halo of the galaxy. Based on the color gradients, there is evidence of moderate star formation activity, with the blue light suggesting the presence of young stars.