The galaxy appears as an elongated, disk-shaped structure, viewed nearly edge-on. A dust lane bisects the galaxy, obscuring a significant portion of the central region and giving it a flattened appearance. The disk exhibits a relatively smooth texture with a slight warp, and the spiral arms are not well-defined. The bulge component seems minimal or non-existent, possibly contributing to the edge-on appearance. The galaxy appears to be undergoing relatively low rates of star formation, based on the overall color and lack of bright, blue star-forming regions. There are no obvious signs of a major merger event, though some minor tidal disturbance cannot be ruled out given the warp. The galaxy likely has a stellar mass on the higher end, based on its apparent size and brightness. It seems to be a typical spiral galaxy observed at a redshift where fine details are beginning to be blurred.
