The galaxy presents as a spiral type, with a disk-like morphology. The spiral arms are well-defined and exhibit a loosely wound structure. Patches of bluer light are present within the spiral arms, suggesting ongoing star formation. A central bulge is visible, appearing moderate in size and brightness relative to the disk. The overall orientation of the galaxy is inclined relative to our line of sight, but not quite edge-on. There are some visual disturbances, indicating a possible minor interaction or past merger event. The presence of a bar structure cannot be confidently confirmed from the image alone, but it may be present. The galaxy is a luminous object and a galaxy of modest mass.