The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. A dominant, roughly spherical central bulge is apparent, with luminosity decreasing gradually toward the outer edges. The color gradient suggests a stellar population that is relatively homogeneous. Some bluer regions could be present along the edges. It is difficult to determine if there are any spiral arms or other distinct features due to the image resolution. There does not appear to be any significant tidal disturbance or signs of an ongoing merger.
