The object presents as a galaxy, likely at a significant distance, given the observed redshift. It exhibits a distinct disk-like morphology, oriented edge-on relative to our line of sight. The central bulge is prominent and appears to be largely spheroidal in shape. The disk component presents a smooth texture, with little indication of distinct spiral arms or significant dust lanes. Color gradients suggest a concentration of older stellar populations within the bulge, while the disk shows evidence of a younger, bluer stellar population. There is no sign of any ongoing major merger, however the presence of minor disturbances cannot be ruled out. The galaxy's overall form is well-defined, without any obvious signs of significant tidal disruption.
