This galaxy presents as a relatively compact object with a smooth, centrally concentrated luminosity profile, indicating an elliptical morphology. There's a dominant, roughly spherical central bulge which appears to be surrounded by a fainter, diffuse halo. The light appears mostly uniform in color, exhibiting a yellowish-red hue, suggesting an older stellar population with minimal ongoing star formation. Close inspection reveals subtle asymmetries and potential minor disturbances in the outer regions, hinting at possible past interactions or mergers. Overall, the galaxy seems to be relatively undisturbed, and a significant portion of the light comes from evolved stars. The redshift indicates that this galaxy is at a significant cosmological distance.
