The galaxy presents as a spiral type, observed at a redshift indicating a relatively close distance. It exhibits a prominent disk structure with well-defined spiral arms visible, though the arms appear somewhat flocculent rather than grand design. The spiral structure suggests ongoing star formation.

The galaxy possesses a noticeable central bulge. The bulge appears moderate in size relative to the disk. No evidence of a strong bar is immediately apparent in the galaxy's morphology. The overall color profile suggests the presence of both older stellar populations in the bulge and younger, bluer stars within the spiral arms. There is no strong evidence of ongoing major mergers or significant tidal disturbances.
