The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth overall appearance. The light distribution exhibits a high degree of radial symmetry, transitioning from a bright, well-defined core outward. This central region displays a yellowish-orange hue, suggesting an older stellar population. There is a lack of clearly defined spiral arms or dust lanes. The outer regions show a gradual decrease in surface brightness, indicating a diffuse halo. Faint blue tinges, near the outer edges, indicate some ongoing, albeit limited, star formation. There are subtle signs of slight disturbance but the overall structure is largely undisturbed.
