The observed galaxy presents as a late-type spiral system viewed nearly edge-on. A prominent central bulge is visible, exhibiting a smooth, rounded morphology. Dust lane obscuration is apparent along the galactic plane, bisecting the galaxy's light. Evidence of spiral arm structure is subtle but suggested by color variations and slight undulations along the disc. The galaxy appears relatively isolated with no obvious signs of tidal interactions or major disturbances. Its redshift indicates a substantial distance, contributing to the observed angular size. The strong red color and smooth, rounded bulge suggest an old stellar population in the bulge. 
