The galaxy presents as a spiral galaxy with a significant disk component. The disk is not perfectly face-on, exhibiting a moderate tilt. This tilt obscures some of the finer details of the spiral structure. The presence of spiral arms is evident, and they appear to be tightly wound around the central bulge.

The central bulge appears relatively small in proportion to the overall disk size, suggesting a later-type spiral galaxy. There is no obvious bar structure visible within the central region. The color gradient suggests that the central region is older and populated by evolved stars, appearing yellower. The spiral arms show hints of bluer regions indicative of ongoing star formation.

There appears to be some asymmetry in the galaxy's structure, potentially indicating minor gravitational interactions or past merger events. There is a slight irregularity or warping of the disk.
