The galaxy presents as a relatively faint, elongated object, likely a spiral galaxy viewed nearly edge-on. A prominent dust lane is visibly bisecting the galaxy's disk, obscuring the starlight and giving it a flattened appearance. The bulge appears to be more rounded than boxy, and the disk exhibits a relatively smooth texture overall. The galaxy's color suggests a population of older stars, with minimal evidence of ongoing, vigorous star formation. There are no signs of major mergers or significant tidal disturbances. The galaxy displays a low rate of star formation, and a relatively moderate mass.
