The galaxy presents as a generally smooth, elliptical-like structure, with a concentrated central bulge region that exhibits a strong reddish-orange hue, possibly indicating an older stellar population and dust obscuration. The galaxy has a round morphology, though there appears to be minor disturbances within the galaxy, that may have been caused by a minor merger or gravitational interaction with another galaxy. There are some feint patches of bluer color, suggestive of younger stellar populations. These patches are not located in the core, and instead make up outer parts of the galaxy. Overall, the galaxy appears evolved and relatively quiescent.
