The galaxy presents as a disk galaxy, viewed almost perfectly edge-on. A prominent central bulge dominates the galaxy's luminosity, appearing smooth and spheroidal. The galaxy is generally yellowish-white in color. The disk component is very thin and relatively smooth, lacking any significant visible substructure such as spiral arms or distinct dust lanes. The outer edges of the disk fade gradually, indicating a smooth transition in stellar density. There is some indication of dust obscuration in the disk, particularly near the central bulge. The galaxy is isolated, with no immediate signs of tidal interaction or ongoing mergers.
