The galaxy exhibits a distinct spiral morphology. The spiral arms are tightly wound and appear to be multi-armed, though their precise number is difficult to ascertain due to image resolution. A prominent central bulge is apparent. The bulge appears moderately sized relative to the disk. There is a subtle bar-like structure extending across the bulge, with an orientation along the horizontal axis.

The color distribution reveals a gradient with a yellowish hue concentrated in the central bulge, transitioning to bluer tones in the outer spiral arms. This suggests ongoing star formation in the disk regions. The overall form of the galaxy appears relatively undisturbed, with no obvious signs of a major merger. However, there is some minor asymmetry in the distribution of light in the disk, possibly indicating a minor interaction or internal dynamical processes. The galaxy is viewed at a relatively face-on orientation, allowing for clear observation of its spiral structure.
