The galaxy presents as a face-on spiral with distinct, though somewhat fragmented, spiral arms. The central bulge appears moderately sized and exhibits a smooth, diffuse texture. Evidence of a bar is not immediately apparent but subtle elongation within the central region may indicate a weak bar structure. Star formation appears ongoing within the spiral arms, indicated by the presence of bluer regions. There are also indications of redder regions that possibly indicate an aging stellar population. No major mergers or significant tidal disturbances are visible, though minor irregularities within the spiral arms hint at possible past interactions. The overall morphology suggests a transitionary stage between a grand-design spiral and a more flocculent spiral structure.
