The galaxy presents a smooth, elliptical morphology, exhibiting a high degree of central concentration. Its overall shape is predominantly round. There are no prominent spiral arms or a well-defined disk structure discernible. Faint color variations are observed, transitioning from a reddish hue in the core to a subtly bluer tinge in the outer regions, possibly indicating a difference in stellar populations and star formation activity across the galactic radius. The image does not reveal any signs of significant tidal disturbances or ongoing merger events.
