The galaxy presents as a centrally concentrated object with a moderate degree of smoothness. There is some indication of a possible minor disturbance or merger event occurring, which is causing some irregularities in its morphology. The object is not perfectly round, but has a noticeable intermediate shape. The core of the galaxy is relatively bright. There is a hint of green/blue tinges in the main disk, which may be indicative of current star formation. There is a very faint red object on one end of the galaxy, as well as a redder area on the side. This may suggest the presence of older stellar populations, or dust obscuration in those regions. The morphology is complex, suggesting a dynamic system possibly undergoing interactions.
