The galaxy presents as a moderately luminous, elliptical or lenticular structure at a redshift indicating a significant distance. It appears to be relatively smooth in texture, lacking prominent spiral arms or distinct dust lanes. The central bulge region is bright and concentrated, exhibiting a slightly yellowish hue, potentially indicative of an older stellar population. Moving outwards from the core, there's a gradual transition into a fainter, more diffuse halo. A hint of bluer light is visible in this outer region, suggesting the presence of some younger stars or ongoing star formation, albeit at a low rate. The overall morphology appears undisturbed, with no clear signs of major tidal interactions or ongoing mergers. The shape is generally rounded, though with a slight elongation along one axis. There's no evidence of a strong active galactic nucleus based on the image alone.
