The galaxy presents a distinct elongated morphology, with a high degree of asymmetry. There is a brighter central region which could indicate a galactic bulge. The overall color of the galaxy is slightly red, potentially suggesting an older stellar population and reduced ongoing star formation. The disk shows some unevenness, indicating possible disturbances. No clear spiral arm structure is observed. The galaxy has a estimated stellar mass on the higher end. Evident from the morphology, the galaxy may be undergoing or have undergone a minor merger event.
