The galaxy presents as a disk-shaped system, viewed almost edge-on from our line of sight. A distinct bulge is not easily discernible; however, the central region exhibits a higher luminosity, implying a concentration of stars toward the galactic center. The disk appears relatively smooth, with no immediately apparent spiral arm structure, and is more luminous towards the center and dims as it reaches the edge. The colour suggests it consists of older, redder stars and possibly a moderate amount of dust obscuration within the disk plane. There is evidence of minor interaction with another object, but it appears to be undisturbed and not merging with another galaxy.
