The galaxy presents as a moderately bright, centrally concentrated object. Its morphology appears largely smooth, with a high degree of radial symmetry. The light profile suggests a spheroidal shape, possibly elliptical. There is a clear color gradient, with a yellowish central bulge transitioning to a bluer outer halo. The absence of strong spiral arm features or dust lanes indicates a relatively undisturbed system. There may be minor perturbations in the outer regions, but they do not suggest an ongoing major merger event. The galaxy displays some evidence of star formation as suggested by the blue color in the halo, but is mostly comprised of older stars. Overall, the galaxy appears to be a relatively massive and luminous system with a redshfit of approximately 0.17.
