The galaxy presents as an edge-on spiral, exhibiting a clear disk structure. A substantial dust lane is visible, bisecting the galaxy's luminous plane and obscuring light from the far side. The bulge appears prominent and rounded, concentrated at the center of the galaxy. Little to no arm structure can be discerned as this is an edge on galaxy. There are no signs of major mergers or significant tidal disturbances. The galaxy has a redder hue when compared to other galaxies that can be seen in the field, suggesting an older stellar population and lower ongoing star formation rate.