The galaxy exhibits a well-defined spiral structure, characterized by tightly wound arms that emanate from a prominent central bulge. The arms are not perfectly symmetrical, displaying some patchiness and irregularities in their distribution. Star formation appears active within the arms, evidenced by the presence of bluish knots which likely correspond to regions of intense starbirth. A subtle bar-like feature seems to extend through the central region, though it is not overwhelmingly dominant. The bulge itself shows a smoother, more uniform color, suggesting an older stellar population. There may be a small amount of dust obscuring some of the arms, based on subtle color variations. Overall, it presents as a relatively face-on spiral galaxy with a notable bulge, active star formation in the spiral arms, and a possible weak bar structure.
