The galaxy presents as an elliptical or lenticular system at a redshift suggesting a significant distance. It exhibits a generally smooth morphology with a high degree of central concentration. Its overall color profile indicates a dominant older stellar population. There is a lack of distinct spiral arm structures or prominent dust lanes visible, suggesting a lower rate of active star formation. The galaxy shows a slight deviation from perfect circularity, hinting at a possible mild tidal interaction or intrinsic ellipticity. There are no signs of major ongoing mergers or significant disturbances. The galaxy appears to be relatively isolated, without obvious nearby interacting companions in this field of view.
