The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution appears fairly uniform throughout the galaxy, with a gradual decrease in intensity from the core outwards. There is a slight elongation visible, suggesting it is not perfectly spherical. A faint, diffuse halo surrounds the central region. There is no prominent evidence of spiral arms or significant dust lanes. The overall color appears yellowish-white, indicative of an older stellar population. There is no obvious sign of intense star formation, although a small amount cannot be ruled out. No significant morphological disturbance, such as tidal tails or asymmetries, is apparent. The galaxy is likely a massive system. 
