The galaxy appears as a concentrated, elliptical-like structure, with a relatively smooth light distribution. Its light appears to be dominantly concentrated in the central region, with a gradual decrease in luminosity towards the outer edges. The color appears mostly yellow-orange throughout, with hints of what appears to be an older stellar population. The round shape suggests a system with little ongoing star formation or significant dust obscuration. There is some subtle evidence of minor disturbances, such as tidal tails, suggesting that there could be minor gravitational interactions influencing its structure. The overall morphology indicates it is likely a massive galaxy that has undergone significant quenching of its star formation.
