The object appears to be a spiral galaxy at an intermediate redshift. The morphology is characterized by well-defined spiral arms, exhibiting a flocculent structure with considerable patchiness throughout. The winding of the spiral arms ranges from tight to loose, showing medium winding as the main component. The central bulge is moderately sized and appears relatively luminous, while the disk component is bluer in color suggesting more recent or ongoing star formation. There is no clear evidence of a strong bar structure. The galaxy does not seem to have any major disturbances due to mergers, but there is some indication of minor interaction or tidal features. The overall impression is that of a well-formed spiral galaxy exhibiting normal star formation within its disk.
