The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The light distribution suggests a mostly featureless structure, characteristic of an elliptical or lenticular galaxy. It appears to be mostly spheroid, though there is a slight elongation, tending towards an in-between shape. The color index indicates a population of older stars, as shown in the redder hues present throughout the galaxy's halo, however there is a population of younger stars towards the center, as shown by the slightly blue-white tint. There is no evident presence of a significant disk or spiral structure, nor any signs of strong tidal interactions or major mergers. 
