The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge that appears yellow-orange in color, suggesting a population of older stars. The light tapers off gradually from the center, with a slight extension along one axis, hinting at a possible disk-like component or tidal feature, though the galaxy is largely featureless. The overall color suggests minimal ongoing star formation, with light being predominately from older stellar populations. There is very slight disturbance, as the shape of the halo around the bright center tapers off more on two sides than the other two. It is a relatively compact object, likely quite massive given its apparent luminosity and lack of significant structure.
