The galaxy presents a discernible spiral structure, although the arms appear somewhat tightly wound. A prominent central bulge is visible, exhibiting a yellow hue, suggesting a population of older stars. The disk component displays a bluer color, indicating the presence of younger stars and ongoing star formation regions. The galaxy is not perfectly face-on, presenting an inclined view. Overall, the galaxy exhibits a classic spiral morphology with a substantial bulge and well-defined spiral arms. No signs of major mergers or significant tidal disturbances are immediately apparent in this image.
