The galaxy presents a distinct spiral morphology. Tight winding is observed in the spiral arms. A prominent central bulge is present, though it appears moderately sized relative to the overall galactic disk. The disk shows no inclination, presented as face on to our viewpoint. Evidence of recent or ongoing star formation is suggested by the relatively blue color. The galactic structure appears relatively undisturbed, and the presence of merging with another galactic body is not evident.
