The galaxy is a disk galaxy, observed edge-on. A prominent dust lane is visible along the galactic plane, obscuring some of the light from the galactic bulge and disk. The bulge appears to be somewhat rounded. The disk exhibits a relatively smooth texture, with no apparent signs of spiral arms. The galaxy color suggests a relatively older stellar population and a modest star formation rate. There are no signs of major disturbances or ongoing merger activity. The galaxy appears to be relatively isolated.
