The galaxy presents as a relatively large, edge-on spiral. A prominent central bulge dominates the morphology, appearing smooth and spheroidal. The outer disk exhibits a relatively flattened profile. There is little evidence of strong spiral arm structure or significant dust lanes within the observable spectrum, with a slight blueish hue along the edges of the disk and a more yellowish hue at the core of the disk. There are no obvious signs of tidal disturbances or interactions with other galaxies, and the galaxy appears relatively undisturbed. The galaxy has a estimated mass above 10^11 solar masses. Star formation activity appears to be very low.
