This galaxy appears to be a relatively face-on spiral galaxy with a prominent bulge. The central region is bright and concentrated, indicative of a dense stellar population, likely older stars. The spiral arms are somewhat tightly wound and appear fuzzy or flocculent, suggesting ongoing but perhaps not exceptionally vigorous star formation. The color of the galaxy is generally bluish-white, especially in the arms, which is consistent with the presence of younger, hotter stars. Some regions appear slightly redder, likely due to dust obscuration or older stellar populations. There might be a subtle bar structure present through the center. Overall, the galaxy appears relatively undisturbed, exhibiting a classic spiral morphology. There is a very slight asymmetry in the disk structure, but no strong evidence of recent major merger activity is visible.
