The galaxy appears to be a disk galaxy, observed nearly edge-on. The central bulge exhibits a bright, concentrated luminosity, indicating a significant population of older stars. Extending outwards from the bulge is a faint, diffuse disk. The light distribution within the disk seems relatively smooth, although some subtle asymmetries and minor irregularities are present, possibly indicative of minor disturbances. There is a subtle color gradient noticeable from the inner bulge outwards; it appears redder in the central bulge and gradually becomes bluer towards the outer disk, which would align with increased star formation in the arms. There's no clear evidence of a bar structure or strong spiral arms. The overall shape seems to be fairly regular and without major distortions.
