The galaxy presents as a luminous, elliptical morphology with a smooth, concentrated central bulge. The color profile exhibits a general yellowish-orange hue, indicative of a population of older stars. There is a subtle disk component, though it appears relatively featureless, lacking prominent spiral arms or dust lanes. The overall light distribution suggests a relatively evolved system, where star formation may be diminished compared to younger galaxies. Some slight irregularities in the shape and outer halo suggest weak gravitational interactions with companion galaxies or past merger events, but the primary structure is still largely undisturbed.