The galaxy presents as a flattened, disk-like structure with a noticeable bulge. The overall color is dominated by a cool, bluish hue, suggestive of recent or ongoing star formation. A central, somewhat brighter region is visible, possibly indicating a galactic nucleus. The disk exhibits a mottled appearance, with hints of spiral arm structure, though these features are not sharply defined. There appears to be a region of increased reddening, possibly due to dust lanes or regions of older stellar populations, visible within the galactic disk. There are no signs of significant tidal disturbances or interactions with other galaxies, but possible minor distortions might be present in the disk's outer regions. Overall, the galaxy appears to be a spiral galaxy with moderate star formation activity and a relatively undisturbed morphology.
