The object appears to be a spiral galaxy, observed at a redshift that places it at a considerable distance. Its disk is oriented approximately edge-on relative to our line of sight. While a prominent central bulge is not immediately apparent, a slightly brighter, concentrated region suggests the presence of a central galactic nucleus. The galaxy exhibits evidence of active star formation, particularly in regions along the visible arms and towards one end, as indicated by the slightly bluer hue in these areas. Some disturbance is also evident in the morphology, and a minor tidal interaction may be occurring as evidenced by slight asymmetry and a faint extension. Overall, the galaxy presents a disk dominated morphology with ongoing stellar birth and some evidence of gravitational interaction.
