The galaxy presents as a disk galaxy observed nearly edge-on. A prominent, spheroidal bulge is observed, displaying a smooth, rounded structure. The disk appears thin and elongated, with a noticeable dust lane or obscuring band running along the mid-plane. There is a slight asymmetry in the overall light distribution along the disk, suggesting potential tidal interactions or past minor mergers. Overall it is a relatively compact, and undisturbed disk galaxy. The colors are consistent with an older stellar population.
