The galaxy presents as a lenticular or possibly spiral galaxy, observed at an oblique angle. A central bulge is evident, appearing smooth and concentrated with a bright, nearly stellar core. The disk appears somewhat diffuse, with a bluer hue that may indicate recent or ongoing star formation. There appear to be slight disturbances to the disk, possibly indicative of a minor interaction or merger event, but also indicative of spiral arms that are somewhat disrupted. Given its morphology and redshift, it's likely a relatively massive system. Overall, the galaxy shows signs of a transition object.
