The galaxy presents as a flattened, disk-like structure, exhibiting a pronounced central bulge. The bulge is a bright, yellowish-orange color, suggesting an older stellar population. The disk itself displays a more diffuse, mottled appearance, with hints of spiral arm structure. These arms exhibit subtle color variations, possibly indicative of differing stellar populations or dust lanes. There is a slight asymmetry in the outer regions of the disk. The galaxy is observed at an oblique angle. The overall morphology suggests it could be a late-type spiral galaxy or possibly an early-type disk galaxy.
