This galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from a central bulge, appearing loosely wound. The bulge itself presents a moderate size relative to the disk. There is a slight asymmetry observed within the disk structure, potentially indicative of a minor gravitational interaction, although it is not strongly disturbed. The central bulge displays a yellowish hue, suggesting an older stellar population, while the spiral arms exhibit a bluer coloration, indicative of ongoing star formation. The galaxy is oriented at a moderate angle to our line of sight, allowing us to clearly resolve its spiral morphology. There is no evidence of a strong bar structure bisecting the central region.
