The galaxy presents as an edge-on spiral, displaying a notable disk structure. The central bulge appears prominent and exhibits a rounded morphology. Within the disk, there are hints of some structure but the resolution prohibits distinct feature identification. There appears to be no obvious signs of ongoing major mergers, although minor disturbances may exist. The color gradient suggests a stellar population that is not uniform throughout the galaxy. There is a redder color toward the central bulge, which may be suggestive of an older stellar population, and a bluer component in the disk. There is no apparent boxy bulge. The overall appearance is consistent with a galaxy at a redshift where detailed morphological features are blurred, but the fundamental edge-on spiral nature is still discernible.
