The galaxy presents as a flattened, disk-like structure viewed at a significant angle. Its central region appears bright and yellowish, possibly indicative of an older stellar population concentrated in the bulge. The outer regions of the disk exhibit a bluer hue, suggesting the presence of younger, hotter stars, and perhaps ongoing star formation within spiral arms. These arms are not sharply defined, giving the galaxy a somewhat flocculent appearance. There is a lack of strong disturbances or prominent features that suggest recent major merger activity. Faint indications of very minor disturbances exist, potentially caused by a small galactic interaction. Overall, the galaxy displays a relatively smooth morphology with only a few small features.
