The observed galaxy presents as a spiral type. The galactic disk is noticeably inclined with respect to our line of sight, appearing close to edge-on. Distinct spiral arm structures are apparent; the arms appear loosely wound. A central bulge is discernible but appears relatively small compared to the overall disk size. The color distribution suggests the presence of both older stellar populations in the bulge (yellowish/orange) and younger, hotter stars in the spiral arms (bluish). Some dust lanes are suspected within the spiral arms, partially obscuring the starlight. The overall structure indicates a galaxy experiencing or having recently experienced some interaction due to apparent disturbances in the arms.
