The galaxy appears as a centrally concentrated spheroid with a smooth, featureless light distribution. There is no evidence of spiral arms or a bar structure. The galaxy exhibits a nearly circular morphology, deviating minimally from perfect roundness. No signs of tidal tails, bridges, or other major disturbances are apparent, suggesting it is not currently undergoing a major merger. There is a slight color gradient observed, transitioning from a somewhat bluer core to redder outskirts, which might indicate varying stellar populations or dust content within the galaxy. Overall, the galaxy's morphology is consistent with an elliptical galaxy at a moderate redshift.
