The galaxy presents as a spiral, exhibiting a disk-like structure. The orientation is approximately edge-on. The galactic bulge appears moderately sized and luminous, with a somewhat amorphous shape. Faint spiral arm structures are suggested, though not sharply defined, and seem to trace a loosely wound pattern within the disk. The color gradient suggests a higher concentration of older stars towards the central bulge, with bluer regions indicating areas of more recent star formation in the disk. Some dust lanes are present, causing patchy obscuration, particularly within the disk region. The galaxy does not obviously display any signs of major merging events or significant disturbances, although some minor irregularities may indicate past interactions.
