The galaxy presents a clear spiral structure. Its arms are well-defined and exhibit a winding pattern, neither tightly wound nor exceptionally loose, presenting an intermediate appearance. The arm count is approximately two, and appears fairly symmetric. The galaxy has a distinct, but not dominating central bulge, with some observed disk prominence. There appears to be a bar structure crossing the center of the bulge. The disk is observed face-on and does not appear to be edge-on. The galaxy appears relatively undisturbed, with no significant signs of major mergers or strong tidal disruptions. The overall color suggests ongoing star formation, exhibiting blue hues. The isophotes appear smooth, with no presence of bright knots suggesting star clusters.