The galaxy presents as a spiral galaxy with a moderate bulge. The bulge region is a yellow-orange color which indicates an older population of stars. There are spiral arms extending from the central region with a blueish tinge, suggesting the presence of younger, hotter stars and ongoing star formation.

There is not a significant amount of dust obscuring the arms. A bar structure is visible in the central region, appearing relatively short but distinct. The spiral arms appear somewhat patchy, indicating an uneven distribution of star formation regions or variations in stellar density. Overall, the galaxy exhibits a well-defined disk structure.
