The object appears to be a spiral galaxy at a considerable distance. The galaxy's disk is oriented approximately edge-on relative to our line of sight. There is a noticeable bulge component, exhibiting a yellowish hue suggesting an older stellar population. Faint, tightly wound spiral arms are visible, and a possible bar structure bisects the central bulge. Star formation appears to be ongoing, as evidenced by the blue tinge along the galactic disk. There are no obvious signs of any major merger event.
