The galaxy exhibits a prominent spiral structure, with well-defined arms that appear somewhat tightly wound. The arms display a clumpy texture, suggesting active regions of star formation. These regions show a bluer color, consistent with the presence of young, hot stars. A central bulge is visible, though it appears relatively small compared to the overall disk size. There's evidence of a possible bar structure bisecting the bulge. The disk is not perfectly face-on, exhibiting a slight tilt. The overall color of the galaxy is intermediate, suggesting a mix of stellar populations, but with a noticeable contribution from younger, bluer stars in the spiral arms. No obvious signs of major recent mergers are apparent.
