The galaxy presents as an edge-on spiral, with a prominent dust lane bisecting the galaxy along its major axis. The bulge appears to be somewhat rounded and exhibits a higher concentration of light, fading outward towards the disk. There are signs of low level star formation activity present, implied from what appears as variations in luminosity and color across its disk and bulge. Faint tidal features or disturbances are present around the disk, suggesting possible recent or ongoing interactions. The galaxy's overall color index indicates the presence of a relatively mature stellar population within the disk. It has a estimated stellar mass of approximately 10^10 solar masses.
