The galaxy presents as a relatively face-on spiral. Its dominant feature is a bright, centrally located bulge. The spiral arms are well-defined and extend outwards from the bulge. They appear tightly wound, displaying a medium pitch angle. Dust lanes are visible within the spiral arms, especially on the upper right quadrant of the galaxy, adding to the arms' structure. The spiral arms exhibit a distinct, patchy distribution of star formation.

The overall color suggests a mixed stellar population, with a significant presence of older, redder stars in the bulge, along with pockets of younger, bluer stars within the arms indicating ongoing star formation. There's a hint of asymmetry in the outer regions of the disk. No obvious signs of a major merger are visible. There appears to be a relatively small, well-defined bulge. The galaxy is relatively smooth. The nucleus is bright.
