The galaxy presents as a single, largely featureless entity. Its morphology is predominantly smooth and elliptical, with a high degree of central concentration. The shape is nearly circular. A subtle color gradient is apparent, transitioning from a yellowish-orange core to a slightly greenish outer halo. This suggests an older stellar population concentrated in the center, possibly surrounded by a younger, bluer population, or dust. No obvious spiral arms or bar structures are visible. There are no signs of active merging events or significant tidal disturbances; the galaxy appears relatively undisturbed. The light distribution appears regular and symmetric, further reinforcing the classification as a smooth system. Overall, the galaxy presents as a well-formed, elliptical system with possible variations in stellar population across its radial extent.
