The galaxy presents as an edge-on spiral, with a prominent, luminous central bulge. The bulge exhibits a smooth, rounded morphology. A flattened disk extends outwards from the bulge, obscuring some of the bulge's light along its plane. There appears to be a dark dust lane running through the middle of the galaxy. There is evidence of star formation in the disk. The galaxy appears largely undisturbed, without significant signs of tidal interactions or major mergers. The galaxy is estimated to be of intermediate mass. The specific star formation rate suggests that it lies in the lower range. 
