The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure with prominent spiral arms. These arms display a grand design, tightly wound around a central bulge. The bulge is relatively small compared to the size of the disk. A strong bar feature extends through the center of the bulge, providing structure and stability to the arms. The spiral arms have a flocculent appearance, indicating ongoing star formation within them. The bluer color in the spiral arms indicates the presence of young, massive stars. The galaxy is relatively face-on, allowing for a clear view of the spiral structure. There does not appear to be a significant amount of dust obscuration in the arms. Overall, this spiral galaxy displays a classical morphology with a well-defined disk, tightly wound spiral arms, and a bar feature, indicative of a dynamic and evolving system.