The galaxy presents a disk-like morphology, viewed at an oblique angle, but not quite edge-on. It exhibits a distinct spiral structure, characterized by multiple arms emanating from a central region. These arms appear somewhat flocculent, displaying clumpy regions that are suggestive of ongoing star formation. The color gradient indicates a higher concentration of younger, bluer stars within the spiral arms, contrasting with the redder hues often associated with older stellar populations. A modest bulge component is apparent, though not particularly dominant within the overall galactic structure. There is some evidence of a central bar-like structure, potentially influencing the spiral arm morphology. There is no obvious signs of tidal distortions or major mergers, although some subtle asymmetry may indicate minor interactions.
