The galaxy presents a flattened, disk-like morphology, observed at an angle that is not quite edge-on but significantly inclined. A central bulge is clearly visible, exhibiting a smooth, concentrated luminosity profile that peaks intensely. The color of this central region appears to be yellowish-white, suggesting an older stellar population.

The galactic disk shows some evidence of structure, though it is not highly defined. There are hints of spiral arm features, but these are faint and somewhat diffuse. The disk's color is bluer than the bulge, indicative of the presence of younger, hotter stars and potential ongoing star formation.

There's a slight asymmetry in the outer regions of the disk, with some indication of a minor disturbance in the galaxy's morphology, but the overall structure is relatively intact. The galaxy doesn't seem to be undergoing a major merger.
