The galaxy exhibits an overall elliptical morphology, appearing largely smooth and somewhat elongated. A bright, concentrated central bulge is evident, displaying a yellowish hue, which suggests a population of older stars. Surrounding the bulge is a fainter, more diffuse halo. Faint hints of what could be a very subtle disk-like structure are present, oriented almost edge-on. No prominent spiral arms or dust lanes are visible, though there may be minor disturbances indicating it could have minor mergers. The relative lack of blue light in the outer regions suggests a low rate of recent star formation. The galaxy is generally round.