The galaxy presents a discernible disk structure, viewed at an angle far from edge-on. Spiral arms are clearly visible, with a tightly wound morphology. Two major arms are very prominent and visible to the eye. A central bulge appears present, contributing significantly to the overall luminosity of the galaxy. The galaxy color displays variations, with a notable yellow-orange hue concentrated within the bulge region, suggesting an older stellar population. Patches of bluer color are observed along the spiral arms, indicative of recent or ongoing star formation. No significant disturbances from recent mergers or interactions with other galaxies can be discerned in the overall galactic structure. The presence of a bar-like structure is somewhat ambiguous, it does not stand out as a particularly dominant feature.