The galaxy presents as a single object with an apparent morphology tending towards smooth. It exhibits a generally circular shape. There is a distinct color gradient across the object, transitioning from a blue-green hue in the upper portion to a more yellow-red hue in the lower portion. The color variation suggests potential differences in stellar populations or dust content across the galaxy. A disruption can be seen towards the bottom of the galaxy suggesting the effects of a merger. These observations suggest the galaxy may be the product of an on-going merger event.
