The galaxy presents as a spiral galaxy with a relatively small bulge. The spiral arms are well-defined and moderately tightly wound, with some arms appearing to branch. The arms exhibit a patchy, flocculent structure with apparent star forming regions. The central bulge appears to have a yellow hue, suggesting an older stellar population, while the arms are bluer, possibly due to ongoing star formation. The galaxy appears relatively undisturbed. The orientation provides a near face-on view of the galactic disk, enabling detailed observation of the spiral structure.
