The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears largely elliptical, approaching a circular morphology. There may be a subtle hint of a disk, but it is not sharply defined. A slight disturbance is also present, as the galaxy is asymmetrical in shape. The galaxy emits strongly in the blue region of the spectrum, implying the presence of a young population of hot, massive stars. There is no obvious structure or morphological feature that indicates a recent or ongoing major merger event.
