The galaxy exhibits an overall morphology that appears to be undergoing a merger or interaction. A dominant central component displays a roughly intermediate ellipticity, neither perfectly circular nor highly elongated. Emanating from this central region are what seem to be tidal features or distorted structures, suggesting gravitational interaction with another galaxy. The core appears relatively smooth in its light distribution. While the galaxy's form is somewhat amorphous, with no defined spiral arms or a clear, regular disk visible. There is a slight blueish-green tint to the galaxy, and this might represent an active region of star formation. There might be some light disturbances in the form of distorted arms. The core of the galaxy is round and smooth.
