This galaxy presents as a face-on spiral, exhibiting a prominent disk structure. Two well-defined spiral arms are readily apparent, winding tightly around the galactic center. The winding of these arms appears relatively uniform throughout their extent.

A central bulge is observed, contributing significantly to the overall luminosity of the galaxy. The bulge is moderate in size, not dominating the disk but clearly present. The color distribution suggests a central concentration of older stars in the bulge, appearing yellower than the bluer spiral arms where active star formation is likely occurring. There is no strong indication of a bar structure within the galaxy.

The overall morphology suggests no signs of recent major mergers or significant tidal disturbances. Minor disturbances cannot be ruled out, though the overall structure appears relatively settled.
