The galaxy appears to be a spiral galaxy, observed at a redshift indicative of a substantial distance. It presents with moderately defined spiral arms, exhibiting a somewhat flocculent structure. A central bulge is prominent and appears to dominate the central region of the galaxy, being fairly large relative to the galactic disk. The disk appears relatively smooth. There is little to no visible evidence of significant recent merger activity, and any tidal features are not apparent. Overall, this spiral galaxy demonstrates a morphology consistent with a relatively mature system, yet retains significant spiral arm structure.
