The galaxy presents as a face-on spiral, exhibiting a generally smooth and oval central bulge. A subtle disk structure surrounds the central bulge, displaying a faint hint of spiral arm morphology. The arms appear somewhat diffuse and poorly defined. There is an even distribution of light. There is an indication of some possible disturbance within the galactic structure. Overall, the galaxy appears relatively undisturbed, with no major signs of ongoing merger activity or strong tidal interactions.
