The galaxy exhibits a disk-like structure, though with some observed irregularities. The overall color suggests the presence of both younger, bluer stellar populations and older, redder populations, which could indicate ongoing or recent star formation within the disk. Spiral arm structures appear to exist but are not sharply defined, showing a somewhat flocculent morphology. A central bulge is present. The absence of strong tidal features suggests no major merger events. The galaxy appears neither completely smooth nor clearly defined as a spiral galaxy, but shows disk-like characteristics.
