The galaxy presents a smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that diminishes gradually towards the outer edges. The color gradient shifts from a yellowish hue in the core to a subtly bluer tone in the outer regions. No distinct spiral arms or bar structures are immediately apparent. There are no prominent tidal features or obvious signs of recent major mergers, although some minor irregularities in the outer regions suggest possible interactions. The overall roundness of the galaxy is notable, deviating minimally from a perfect circle. The luminosity indicates a relatively massive system, suggesting a high likelihood of hosting a supermassive black hole at its center. Star formation seems to be occurring at a modest rate.
