The galaxy presents as a spiral, likely at an oblique angle relative to our line of sight. It exhibits prominent spiral arms, with a generally tightly wound morphology. A bulge is present within the galaxy's core, appearing moderate in size compared to the overall galactic disk. A bar may be present running through the central bulge, it is difficult to clearly resolve. There are areas of active star formation occurring in areas along the spiral arms, visible as enhanced brightness and color variation. There is no immediately apparent interaction or major disturbance affecting the overall structure, although subtle indications of minor disturbances or past interactions cannot be ruled out based on this image alone.
