The galaxy presents a clear spiral structure. Multiple spiral arms are observed emanating from a central bulge. These arms exhibit a range of winding tightness, appearing primarily medium to tightly wound. Patches of bluer light are seen along the spiral arms, indicating regions of active star formation. The central bulge shows a more yellowish color, potentially suggesting an older stellar population. The galaxy appears inclined to our line of sight, allowing a clear view of the spiral arm structure. There is some asymmetry and distortion to the structure, possibly indicating a minor gravitational interaction or disturbance. There are also some hints of a bar structure in the center.
