The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms appear moderately wound, with a patchy distribution of star-forming regions visible as subtle color variations, particularly in bluer hues. The central bulge is relatively small and presents a smooth, concentrated light profile. The overall disk appears somewhat disturbed, possibly indicating a minor gravitational interaction or recent merger event, though no distinct companion galaxy is immediately apparent. A faint bar structure may be present, although it is not distinctly pronounced. The galaxy is viewed at a moderate inclination angle.
