The galaxy presents as a face-on spiral, exhibiting a distinct morphology. The central bulge appears moderately sized and luminous. Two prominent spiral arms wind tightly around the core, showing evidence of star formation regions which are noticeably blue in color. These arms display a fairly symmetrical structure. It appears that there may be a bar-like structure, or the hint of one, in the central region. There is no significant evidence of major mergers or substantial tidal disturbances, though a small perturbation can not be ruled out.
