The galaxy presents as a well-defined spiral structure with a prominent central bulge. The spiral arms appear tightly wound and relatively smooth, suggesting a grand design spiral galaxy morphology. The bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms display a bluer color, implying the presence of younger, hotter stars and ongoing star formation. Dust lanes are faintly visible within the spiral arms, obscuring some of the starlight. The galaxy exhibits no obvious signs of significant tidal disturbance or ongoing merger activity. The overall appearance suggests a relatively undisturbed and evolved spiral galaxy.
