The galaxy presents as an edge-on spiral, exhibiting a distinct dust lane bisecting the central bulge. The bulge appears prominent and well-defined. The disk shows a relatively smooth structure with little evidence of strong star formation regions. It has a median size of a few kiloparsecs. The galaxy's color suggests an older stellar population, indicative of a low specific star formation rate. No strong signs of interaction or merging events are immediately apparent, although there may be minor disturbances in the disk. The bulge appears to be more rounded in shape. The dust lane is thin, with a prominent bulge.