The galaxy presents as a singular, smooth, and relatively round object with a concentrated core. There is a slight elongation, but the overall shape is largely spheroidal. The light distribution appears fairly uniform and diffuse. The system displays a distinct double nucleus or a galaxy merger in its final stages. The color is yellowish with no substantial blue components evident, suggesting a population of older stars and limited ongoing star formation. Some faint disruption in the general structure of the light around it seems to be apparent.
