The galaxy presents as a system of several distinct luminous components. There is no obvious spiral structure, suggesting the galaxy is most likely elliptical in nature or a highly inclined spiral galaxy. The dominant light is yellowish-red, typical of older stellar populations, implying relatively low levels of ongoing star formation. The smooth appearance and relatively round shape supports its classification as an elliptical galaxy. Some disturbance or interaction may be present, although the limited resolution and depth of the image make this determination uncertain. Overall, it appears to be a relatively massive, evolved galaxy, possibly undergoing minor interactions.
