This galaxy presents as an edge-on spiral or lenticular galaxy, exhibiting a flattened disk structure viewed almost perfectly from the side. The galactic bulge appears relatively small and slightly elongated along the major axis, suggesting it might be more akin to a pseudo-bulge. There is no strong evidence of a classical bulge. The disk itself shows minimal indication of spiral arm structure or dust lanes, appearing fairly smooth and uniform in color. The color is slightly blueish, implying the presence of some younger stars, but this is subtle. There is no obvious evidence of active star formation regions. The galaxy seems relatively isolated, with no nearby interacting companions discernible.
