This galaxy appears to be a spiral galaxy, viewed nearly edge-on. A central bulge is visible, appearing yellowish in color. The disk component extends outwards from the bulge, showing a slight bluish tint, possibly indicating the presence of younger stellar populations and ongoing star formation within the galactic disk. The morphological classification suggests that the galaxy is relatively undisturbed, without strong evidence of recent or ongoing major mergers. The relative smoothness and coherent shape are consistent with a non-interacting, evolving system at its redshift.
