The galaxy presents as a spiral, exhibiting a notable disk structure viewed at a moderate inclination. A central bulge is apparent, though it appears relatively small compared to the overall size of the disk. The spiral arms are prominent and exhibit a tightly wound morphology in the center. The color suggests active star formation regions within the arms, indicated by a bluish hue along their length. No dust lanes are clearly discernible. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major merging activity or tidal disruptions.
