The galaxy presents as a spiral type, with a clear disk structure. The spiral arms are well-defined, exhibiting a two-armed structure. The arms appear somewhat tightly wound closer to the center, becoming more open as they extend outwards. Within the spiral arms, there are hints of star-forming regions, evidenced by subtle color variations that suggest the presence of younger, bluer stars in these areas.

The galaxy features a prominent bulge, though it does not appear to dominate the overall structure. A stellar bar is visible traversing the central region, which influences the structure of the inner spiral arms.

There is a slight asymmetry observed in the disk, possibly due to minor gravitational disturbances or interactions. The overall structure suggests a galaxy that is not undergoing a major merger, although minor disturbances might be present.
