This galaxy presents as a moderately bright, elongated object. It exhibits a relatively smooth, concentrated central bulge that appears slightly brighter than the surrounding regions. The disk appears lenticular, with a lack of well-defined spiral arms. The galaxy appears flattened with an approximate axis ratio of 0.6. There is a subtle color gradient across the galaxy, the central bulge appears slightly redder than the disk. There is no clear evidence of major ongoing mergers or tidal disturbances, although the possibility of minor interactions cannot be ruled out. Overall, the morphology indicates a relatively evolved system.
