The galaxy presents a generally smooth morphology, exhibiting an elliptical or lenticular form. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus or bulge. The galaxy shows a gradual decline in surface brightness from the core outwards. The overall color suggests a population of older stars, possibly with ongoing, but low-level star formation. There are some minor disturbances or asymmetries visible in the galaxy's outer regions that may indicate a past merger or interaction with another galaxy, although the galaxy appears relatively undisturbed in the current observation. The object displays an apparent roundness to its overall structure, indicative of a system that has settled into a dynamically relaxed state, or is still in the process of forming.
