The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears yellowish-orange in color, suggesting a population of older stars. The outer regions of the galaxy appear more diffuse and somewhat bluer, hinting at a younger stellar population and possibly ongoing star formation, though not at a rate sufficient to disrupt its overall smoothness. There is a slight asymmetry to the shape of the galaxy. There are very minor disturbances in the galaxy. It has a more rounded shape than elongated.
