This galaxy exhibits a somewhat irregular morphology, likely a spiral. There is a bright, concentrated central bulge, suggesting an older stellar population in the core. The presence of bluer hues extending outward from the central region indicate ongoing star formation within the galactic disk. The outer regions appear somewhat disturbed, with a hint of arm-like structures, though not clearly defined. There is a potential interaction or merger occurring with another object, evidenced by the asymmetries and deviations from a regular spiral shape, as well as the reddish color on opposite sides. The smooth fraction is low, suggesting non-negligible amounts of structure.
