The galaxy presents as a largely featureless elliptical. It exhibits a smooth, concentrated central bulge that emits strongly in the g, r, and z bands, indicating a likely population of older stars dominating the core. Fainter and more diffuse light extends outwards in an elliptical shape. The light from the elliptical bulge is predominantly yellowish-white, possibly indicative of an older stellar population with lower rates of star formation. There is little evidence of spiral arm structure, dust lanes, or irregular morphology. The galaxy appears relatively undisturbed with no signs of ongoing merger activity. The shape is slightly elongated, with an ellipticity of about 0.9, but is mostly round. The red shift indicates that this galaxy is a significant distance away, though no clear evidence of active galactic nuclei is present. The galaxy's overall appearance suggests it is a mature elliptical galaxy with a passively evolving stellar population.
