The galaxy exhibits a disk-like morphology with a somewhat disturbed appearance. It displays faint spiral arm structures, with some regions appearing bluer, suggesting areas of active star formation. The central bulge is either small or non-existent. There are indications of potential minor tidal disturbances or even a possible ongoing merger event, as the overall shape is somewhat irregular. The galaxy shows a mix of smooth regions and more textured areas, consistent with the presence of both older stellar populations and younger, star-forming regions. Dust lanes are not clearly visible, though subtle variations in color and brightness suggest their presence. The overall color index indicates that this is a relatively active galaxy with a substantial population of young stars.
