The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is elliptical or spheroidal, appearing quite rounded in shape. There is a very slight elongation, however it is quite minor.  The light profile appears uniform and there is little evidence of spiral arms or significant disk-like features.  There are no apparent major disturbances in its structure that would suggest ongoing major merger activity or tidal interactions.  Based on the light properties, there is likely a large population of older stars. The galaxy displays a slight colour gradient, appearing somewhat bluer near the center and redder in its outer regions.
