The galaxy appears as a lenticular or possibly a spiral galaxy seen at an oblique angle. The galaxy exhibits a smooth light distribution, suggestive of a dominant bulge component. There is some indication of a faint, disky structure, though it is difficult to discern distinct spiral arms due to the viewing angle and the galaxy's overall morphology. The galaxy's color is predominantly yellow-white, which likely indicates a stellar population composed of older stars with only modest ongoing star formation. The galaxy's axial ratio indicates it is not perfectly round, but rather somewhat elongated. There is no strong evidence of significant tidal disturbances or ongoing major mergers based on the smoothness of its overall form, though some minor asymmetries or faint features could be present. The galaxy has a moderate size and luminosity.
