The galaxy presents as a centrally concentrated elliptical system. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. A gradual decrease in light intensity is observed moving radially outward from the core. The overall shape approximates a rounded structure, with a slight elongation, though not definitively cigar-shaped. There are no clearly discernible spiral arms or significant disk-like features. No major merger events are apparent, and the overall structure appears relatively undisturbed, although there might be a very slight disturbance in its morphology.
