The galaxy presents as a spiral galaxy with well-defined, prominent spiral arms. The arms appear to be moderately wound, neither tightly coiled nor exceptionally loose, but display a noticeable winding pattern. The central bulge is moderately sized, contributing a significant but not dominant portion to the overall luminosity of the galaxy. It shows a subtle bar structure. The spiral arms exhibit a bluer hue, suggesting active star formation. There is no evidence of any major merging events. There is a minor disturbance but not a fully fledged merging event. It is mostly unperturbed.
