The galaxy presents as a spiral type, with a relatively bright central bulge. The arms are distinct but somewhat flocculent, displaying a predominantly two-armed structure. The winding of the spiral arms appears to be moderately open. There is some evidence of star formation within the arms, indicated by the presence of bluer regions. A slight distortion in the overall morphology suggests a possible interaction or minor disturbance. A faint bar structure may be present in the central region, though it is not strongly defined.
