The galaxy presents as a face-on spiral, exhibiting a distinct, though not overwhelmingly dominant, barred structure. The bar appears relatively strong and well-defined. The spiral arms are prominent, with a multi-armed structure where a majority show two spiral arms that wind moderately tightly around the galactic center. The arms are somewhat flocculent and appear patchy in color, suggesting ongoing star formation regions along their lengths.

The central bulge is of moderate size relative to the disk, appearing neither overly large nor negligible. Star formation seems to extend into the inner regions of the galaxy, even close to the bulge. The galaxy does not appear to be undergoing any major merging activity, but there seems to be a possible minor disturbance within one arm, and evidence of it slowly undergoing a merging. The disk is viewed nearly face-on.
