This galaxy exhibits a prominent, moderately sized bulge, suggesting a significant population of older stars concentrated towards its center. Fainter spiral arms appear loosely wound and somewhat patchy, hinting at ongoing star formation. The disk is inclined relative to our line of sight. The overall color profile indicates a mixture of stellar populations, with the central bulge appearing more yellow-red, suggesting older, cooler stars, while the disk regions display bluer hues, possibly indicating the presence of younger, hotter stars within the spiral arms. There are some hints that there may be a faint stellar halo extending beyond the main disk of the galaxy.
