The galaxy presents as a relatively smooth, disk-shaped structure. It appears to be viewed at a high inclination, close to edge-on. There is evidence of a central bulge, exhibiting a concentration of light towards the galactic nucleus. The overall color is somewhat redder, suggesting an older stellar population, with lower levels of star formation. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There might be minor disturbances. The galaxy's light is moderately extended, inferring a considerable physical size.
