The object presents as a relatively smooth, elliptical galaxy. Its morphology is characterized by a bright, diffuse central bulge exhibiting a yellow hue. This suggests a population of older stars dominating the core. Extending outwards from the bulge, a faint, slightly elongated halo is observed, showing a subtle greenish tint. This could indicate the presence of some ongoing, though subdued, star formation, or a population of younger stars compared to the bulge. Overall the light appears smooth with no visual distortions. There is no evidence of tidal tails or other clear signs of recent or ongoing merger events.
