The galaxy presents as a spiral type, exhibiting a disk-like structure with evident spiral arms. A central bulge is apparent, though not overly prominent, giving the impression of a moderate-sized bulge relative to the overall galactic disk. The disk is not perfectly edge-on, allowing for a clear view of the spiral structure.

The spiral arms appear tightly wound in sections, with other sections appearing more medium wound. Two dominant spiral arms are observed extending from the central region. The image suggests the presence of a bar structure crossing the galaxy's center. The bar seems to be a strong feature within the galaxy's morphology.

Evidence suggests that the galaxy might be undergoing minor gravitational interaction or a minor disturbance; the arms show some asymmetry.
