The galaxy presents as a spiral type, exhibiting a pronounced disk structure viewed at a moderate inclination. The central region displays a relatively moderate bulge component, less luminous than the surrounding disk. Two distinct spiral arms are readily apparent, exhibiting a medium winding pattern emanating from the central region, with some arm sections appearing looser. There is a strong suggestion of a bar structure crossing the galactic nucleus. The spiral arms show a mottled texture indicating areas of active star formation. No strong evidence of a recent or ongoing major merger is observed, though minor disturbances or tidal features cannot be entirely ruled out. Overall, the galaxy appears well-defined with moderate complexity.
