The galaxy presents as a spiral, viewed at an angle that is neither face-on nor edge-on. Two prominent spiral arms appear to originate from a central bulge. The arms are moderately wound and exhibit a somewhat flocculent structure, with regions of enhanced brightness likely indicative of ongoing star formation. The color of the spiral arms appears bluer than that of the central bulge, suggestive of a younger stellar population in the arms. A weak bar structure may be present in the central region. The galaxy's morphology could be described as showing signs of minor disturbance. The central bulge is moderately sized.
