The galaxy exhibits a morphology that can be described as possessing both smooth and featured characteristics. A significant portion of the galaxy appears as a diffuse, smooth component, potentially indicative of an elliptical or lenticular galaxy. However, there's also evidence of disk-like features or spiral arms, though not clearly defined.

There appears to be some level of disturbance present in the galaxy, and its classification as a merging system is uncertain. It is likely that the galaxy is currently undergoing either a minor disturbance or perhaps a merger event of some magnitude.
