The galaxy presents as an edge-on spiral, displaying a prominent dust lane bisecting the galactic plane. The central bulge appears substantial and elongated, with a boxy shape. The disk exhibits a smooth, relatively featureless morphology, showing a uniform distribution of light. The galaxy shows a slight orange/red hue, implying a stellar population dominated by older stars. There is no obvious sign of active star formation regions within the disk or bulge. There are no signs of any major galactic mergers, but there appears to be a very minor tidal disturbance visible.
