The galaxy presents as a generally smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, indicative of a substantial stellar population or potential active galactic nucleus. The overall color appears red-shifted, with a pronounced yellowish-orange hue. There is little apparent structure outside of the main body of the galaxy, with no obvious spiral arms or distinct features discernable. A very slight asymmetry suggests a potential minor disturbance or past interaction, although the general smoothness dominates. The overall roundness, tending towards elliptical shape, and color suggest an older stellar population with potentially low ongoing star formation.
