The galaxy exhibits a spiral morphology with a moderately sized bulge. The spiral arms are tightly wound around the galactic center. There is no obvious presence of a strong bar feature bisecting the bulge. The disk shows a bluer hue, suggestive of ongoing star formation. The galaxy is not edge-on. There are no visible signs of an ongoing major merger or significant tidal disturbances, though subtle asymmetrical features hint at possible minor interactions. The galaxy appears relatively isolated with no immediate companion galaxies causing apparent gravitational distortion.
