The galaxy presents as a spiral galaxy exhibiting a moderate to tightly wound spiral arm structure. The arms emanate from a central bulge, which appears to be of moderate size relative to the disk. The disk is observed nearly face-on, showing little to no evidence of being edge-on. The central bulge has a smooth appearance, decreasing in intensity toward the outer regions of the galaxy. While there is a relatively symmetric distribution of light, there appears to be some asymmetry within the arms. There is no clear indication of a strong central bar structure, though a weak bar cannot be ruled out. There are possible signs of some recent star formation, and there do not appear to be any signs of major disturbances or ongoing mergers.
