The galaxy presents as a spiral type, viewed at an oblique angle, though not quite edge-on. The structure exhibits well-defined spiral arms emanating from a central bulge. These arms appear somewhat tightly wound, suggesting a later Hubble type. A strong bar is visible cutting through the central bulge. The bulge appears to be of moderate size compared to the galaxy as a whole. The disk component of the galaxy is prominent and shows some internal structure, and the system overall is not undergoing any major mergers, and no sign of major disturbance, or features suggest there is no ongoing merger.
