The galaxy presents as a flattened, disk-like structure viewed nearly edge-on. There is a prominent central bulge exhibiting a yellowish hue, which suggests a concentration of older stellar populations. The disk appears relatively smooth, with subtle color variations indicative of differing stellar populations or dust distribution. The outer regions of the disk display a bluer tinge, potentially indicative of younger, hotter stars or ongoing star formation. No distinct spiral arm structures are discernible given the edge-on orientation. The overall morphology is suggestive of a late-type spiral or lenticular galaxy.
