This galaxy presents as an edge-on spiral system. The central bulge is prominent and appears to be largely spheroidal in shape with a smooth distribution of light. The disk component is very thin and elongated, displaying a slight warp along its major axis. There is a noticeable dust lane bisecting the galaxy along its equatorial plane, obscuring light from the bulge. The color gradient suggests older stellar populations are concentrated towards the central regions as indicated by the redder hue and younger, bluer stars are more dispersed throughout the disk. There is no prominent star formation or bright knots of ionized gas visible suggesting a relatively low star formation rate. There are no obvious signs of tidal disturbances or ongoing mergers suggesting it is an isolated system.
