The galaxy presents as an edge-on spiral system. A prominent dust lane is observed bisecting the galactic disc, obscuring the central bulge region. The bulge itself appears to be small and elongated perpendicular to the disc, possibly indicating a pseudo-bulge or bar structure. The overall color of the disc is yellowish-white, suggesting an older stellar population. The disc exhibits a smooth texture without any readily apparent resolved star-forming regions. The extent of the galaxy appears compact, with a relatively high surface brightness. There is no sign of on-going major mergers, but potentially minor tidal features could be present.
