The galaxy presents as a face-on spiral type. Two prominent spiral arms are visible, displaying a loose winding pattern. A bar structure is indicated, with a moderate presence across the galactic center. A small bulge is observed in the center of the disk. The disk component appears dominant. There is evidence of a possible minor disturbance or interaction, however, no major merger or significant tidal features are apparent. Based on the color and arm structure, the galaxy is actively forming stars.
