The galaxy presents as a spiral type, with a moderate-sized central bulge. Two main spiral arms appear tightly wound, tracing a relatively organized pattern. A bar structure is faintly visible bisecting the central bulge region. The disk component demonstrates significant star formation, evidenced by the clumpy distribution and color variation within the arms. There is no obvious presence of a strong tidal disturbance or major merging event, though a minor interaction cannot be ruled out.
