The galaxy presents as a relatively compact and elliptical structure. It displays a smooth, concentrated light profile indicative of an early-type morphology. The primary color appears greenish, suggesting a moderate level of ongoing or recent star formation. The absence of prominent spiral arms or distinct disk features supports its classification as an elliptical galaxy. There is a very slight irregularity in the shape, suggesting a possible past minor interaction or merger event, though this is not immediately obvious. The overall symmetry and central condensation of light argue against any recent major mergers.
