The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated light profile. The core region is bright and has a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with no clear indication of spiral arms or distinct features typically associated with disk galaxies. There is a slight asymmetry in the outer halo, with a hint of a tidal tail or minor disturbance on one side, indicating a possible past interaction or ongoing accretion event. The galaxy has a moderately high redshift, indicating it is a significant distance away.
