This galaxy appears to be a spiral galaxy, observed nearly face-on. The central bulge is prominent and has a yellowish hue, suggesting a population of older, redder stars. The disk surrounding the bulge exhibits spiral arm structure, although the arms appear tightly wound and somewhat indistinct. The overall color of the disk is a mix of blue and white, indicating the presence of younger, hotter stars, potentially within star-forming regions. There is no readily apparent dust lane or strong evidence of a bar structure within the galaxy. The galaxy's overall morphology appears relatively undisturbed, with no clear signs of a major merger or significant tidal interactions.
