The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall shape is somewhat elongated, transitioning between round and cigar-shaped. There is a slight indication of a disk-like feature, though it is not prominent. A subtle color gradient exists, with a bluer hue towards the outer regions of the disk and a generally redder tone for the central bulge. The galaxy does not exhibit any obvious signs of major disturbances or ongoing merger events. The light distribution suggests a relatively uniform stellar population across the central region.