The galaxy presents as a relatively smooth, elliptical form. Its central region appears as a concentrated and bright, yellowish core. A diffuse halo extends outwards, fading into the background sky. The shape is elongated, and a subtle color gradient is observed from the center towards the outer regions. There is no apparent evidence of spiral arms or a distinct disk. No clear signs of major mergers or significant tidal disturbances are observed, and the galaxy appears relatively undisturbed. The light distribution suggests a dominant bulge component. The galaxy has a low rate of star formation.
