The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Its morphology suggests a prominent disk structure, evidenced by the spiral arms visible. The galaxy has a strong central bulge, with a diameter of approximately one-third of the galactic disc. The spiral arms appear tightly wound around the center, with a noticeable presence of young, blue stars tracing these spiral arms. There appears to be at least two clearly defined spiral arms. There is no visible bar feature. There is no morphological evidence of recent or ongoing major mergers, though a slight asymmetry in the outer regions might indicate minor gravitational interactions or disturbances.
