The galaxy presents a largely smooth, elliptical morphology. It appears relatively round, displaying a high degree of central concentration. The central region exhibits a bright, slightly yellow-white luminosity, gradually fading toward the edges. There is no apparent disk structure, spiral arms, or significant dust lane features visible. The overall structure suggests a mature system without signs of recent major mergers or substantial star formation activity. Faint hints of what could be a very slight disturbance are present, but the galaxy appears undisturbed.
