The galaxy presents a largely smooth, elliptical morphology. There is a distinct central bulge that is luminous, with color suggesting an older stellar population and little ongoing star formation. The galaxy is mostly round but it appears to be slightly elongated. There are no visible spiral arms or prominent dust lanes; the overall structure appears quite homogenous. The galaxy exhibits a diffuse halo extending outwards from the central region, fading gradually into the background. No signs of tidal disturbances or ongoing mergers are apparent.
