The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. The spiral arms are tightly wound, exhibiting a flocculent structure. While difficult to discern precisely, the galaxy appears to have two spiral arms. The disk component of the galaxy dominates its overall appearance. There does not appear to be a strong bar-like structure within the central region of the disk. There are no signs of a major merger. There may be a minor disturbance in the galaxy shape, perhaps due to a past interaction.
