The galaxy presents as a spiral type, with a relatively small bulge component. There is a distinct disk structure present, exhibiting prominent spiral arms. These arms appear somewhat flocculent and disorganized, indicating ongoing star formation. The central region is comparatively bright, but not overly dominant, suggesting a modest active galactic nucleus (AGN) or a high concentration of stars in the bulge. The galaxy is generally blue, indicative of a younger stellar population and continuing active star formation. There is no obvious evidence of a strong bar structure or major merger event, however, there is a possibility of minor disturbances in the structure, perhaps due to a past interaction. Overall, the galaxy is actively forming stars.
