Morphology of the spectroscopically confirmed cluster memberss. Left: Morphology class distribution of the 107 spectroscopically confirmed cluster members from Noirot et al. (2018), shown on the left. The classes are: Disk (1), Spheroid (2), Irregular (3), Compact (4), Unclassifiable (5). Most of the members are disks, however there are large percentages of star-forming spheroids and compact galaxies. Right: Morphology class distribution of the members that have ground-based photometry is shown on the right. The blue and red lined histograms correspond to active and passive galaxies, respectively. The passive LTG are galaxies with star formation rates below the field main sequence.