The galaxy presents an overall elliptical morphology, elongated along its major axis. It has a centrally concentrated brightness profile, appearing smooth. There is a slight bluing. Overall, the galaxy appears to be undergoing relatively low levels of star formation. There is no apparent disk structure, or spiral arms, and the galaxy appears largely undisturbed, with no obvious signs of a major merger event. The color suggests it is composed primarily of older stellar populations. The lack of prominent dust lanes or other features suggests the system is relatively quiescent.
