The galaxy exhibits a distinct spiral structure with relatively well-defined arms. These arms appear somewhat flocculent, displaying numerous star-forming regions characterized by a blueish hue. The central bulge region presents a yellowish-white color, indicating an older stellar population. The size of the bulge appears to be relatively moderate in relation to the disk. There is no strong evidence of a bar structure bisecting the bulge. The disk appears to be oriented at a slight inclination relative to our line of sight. I don't see any major disturbances to the galaxy shape, although there appears to be a slight irregularity in one of the spiral arms. The overall morphology suggests that the galaxy is undergoing active star formation within its spiral arms, while the central bulge exhibits a more quiescent stellar population.
