The galaxy presents as an elongated, edge-on spiral with a high degree of inclination relative to our line of sight. The central bulge appears somewhat prominent and moderately bright, exhibiting a yellowish-white color gradient. Extending outward from the bulge is a relatively thin, elongated disk structure. The disk displays a mottled appearance with hints of dust lanes, contributing to an irregular color distribution along its length. One side of the disk is slightly brighter and appears to have some star forming regions, as hinted by the blue-ish color. No major signs of tidal disturbances or ongoing mergers are readily apparent, though some subtle asymmetries in the disk's structure might indicate a past interaction.
