The galaxy displays a prominent spiral structure. The spiral arms are well-defined and extend outwards from a bright, centrally located bulge. The winding of these arms appears relatively tight, with a hint of multiple arm structures. There is a small, yet noticeable bulge dominating the core. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions, however, there may be minor disturbances and the galaxy appears to be relatively flat. There is a strong presence of blue light and several areas of active star formation.

