This galaxy exhibits a clear spiral morphology. The spiral arms are well-defined, although some segments are less distinct, exhibiting a somewhat flocculent character. The winding of the spiral arms appears to be intermediate, neither tightly wound nor significantly open. Two primary arms appear to emanate from the central region, with hints of additional arm structures branching off. The galaxy's disk is presented face-on, as no significant obscuration or edge-on features are apparent. 

A moderate-sized bulge is visible at the center of the galaxy, contributing significantly to the overall light distribution of the core region. This bulge presents a smoother texture compared to the more patchy structure of the disk and arms. There are no apparent signs of a strong central bar, but a subtle, elongated feature suggests the presence of a weak bar structure.

Overall, the galaxy does not exhibit signs of major mergers, but some asymmetries in the spiral arm structure and subtle distortions in the overall shape hint at minor gravitational interactions or disturbances. Star formation regions, are present within the spiral arms, indicated by brighter, bluer patches. The general color profile suggests a mixed stellar population within the galaxy.
