The galaxy presents a disk-like structure viewed at an intermediate angle, suggesting it is neither face-on nor edge-on. A central bulge component is clearly visible, appearing moderately sized relative to the overall disk. Faint, tightly wound spiral arm structures are visible in the disk with notable star formation activity occurring within these arms. This indicates ongoing star formation within the galaxy. There is a bar structure that crosses the galactic center. The overall color of the galaxy suggests a mix of stellar populations, with a yellowish hue in the central region, possibly indicating older stars, and slightly bluer hues in the outer disk, consistent with the presence of younger, hotter stars in the spiral arms. The galaxy appears relatively undisturbed, with no major signs of recent mergers or tidal interactions.
