The galaxy presents as a smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a diffuse halo extending outward. The core region appears to be comprised of primarily older stellar populations, exhibiting a yellowish-white hue. There is a slight asymmetry, or possible faint disk component, with some bluer color on one edge, which may indicate a small amount of on-going star formation. Overall, it appears to be a relatively quiescent galaxy with minimal signs of active galactic nuclei activity or significant recent merger events. The galaxy exhibits a moderate redshift, indicating it is at a considerable cosmological distance. The approximate physical size is around 5 kpc. The estimated mass of the galaxy is around 10^10 solar masses, with a low rate of star formation activity.
