The galaxy presents as a moderately bright, lenticular system with a redshift indicating a significant distance. It exhibits a relatively smooth, centrally concentrated morphology, indicative of an evolved stellar population. A distinct, elongated shape is visible, though the disk appears somewhat obscured or disturbed. There is a notable asymmetry, possibly due to tidal interactions or a recent minor merger event. The color appears generally redder, consistent with a lower rate of star formation. Evidence suggests it is a massive galaxy with a substantial stellar mass content. The surrounding halo appears diffuse.