The galaxy presents as a spiral type, observed at a moderate redshift. The galaxy displays a noticeable central bulge that appears relatively prominent. The spiral arms are well-defined, exhibiting a tightly wound structure, with two clearly discernible arms. There is no evidence of a strong bar feature in the galactic center. The disk is observed face-on, with a substantial active galactic nucleus with some star formation. There are no obvious signs of major mergers or significant tidal disturbances. 
