The galaxy presents as a grand design spiral, observed at an angle that reveals significant disk structure but is not perfectly face-on. Two prominent spiral arms emanate from a bright, somewhat diffused central bulge. The arms are well-defined, tracing a moderate pitch angle, with what appears to be ongoing star formation occurring along these arms, indicated by slightly bluer patches. The spiral arms exhibit a fairly consistent winding tightness throughout their visible extent.

The bulge appears relatively small compared to the overall size of the galaxy, and shows no signs of being a classical elliptical bulge. There appears to be a stellar bar structure bisecting the bulge region. The bar is pronounced, spanning a substantial fraction of the bulge diameter.

The disk appears generally undisturbed, with no obvious signs of tidal interactions or major mergers. The overall color index suggests a moderate population of young stars and ongoing star formation within the disk.
