The galaxy presents as a centrally concentrated object, appearing largely smooth in texture. It exhibits a generally elliptical morphology, with a round profile. There may be faint hints of spiral structure, however the general appearance seems to resemble an early-type galaxy. There is a very slight disk component to the galaxy, which is almost face-on. No obvious signs of major merger activity are noted, but there is an extremely minor disturbance nearby. Color gradients suggest a central concentration of older stellar populations, and some limited ongoing star formation. The galaxy is of considerable size and mass.
