This galaxy presents as an elliptical system exhibiting a smooth, concentrated light profile. The morphology appears largely spheroidal with high degree of central concentration. The color is consistent with an evolved stellar population, with redder tones dominating. There is little indication of a distinct disk component or spiral arm structure, nor is there any evidence of active star formation within the visible portion of the galaxy. The system exhibits a relatively undisturbed morphology, with no obvious signs of ongoing mergers or tidal interactions. A compact and centrally located bulge-like structure is evident, surrounded by a fainter, more diffuse halo-like component. Based on its apparent redshift, this galaxy is situated at a considerable cosmological distance.
