The galaxy presents as a flattened, elongated object, strongly indicative of a disk galaxy viewed nearly edge-on. A prominent central bulge is visible, displaying a concentrated, yellowish-orange hue that suggests an older stellar population. The disk component exhibits a bluer coloration, hinting at ongoing star formation regions. There is a slight asymmetry, possibly due to gravitational interaction, but the majority of the galaxy appears relatively undisturbed. The high edge on fraction supports this galaxy is mainly a disk. Overall, the galaxy exhibits characteristics consistent with a massive spiral system at moderate redshift.
