This galaxy exhibits a distinct spiral structure, although the arms appear somewhat flocculent and not sharply defined. A central bulge is present but not especially prominent, suggesting a relatively late-type spiral morphology. There's a suggestion of a bar-like structure crossing the bulge. The overall color profile leans toward the blue end of the spectrum, hinting at ongoing star formation within the galaxy. There may be a slight interaction or minor disturbance as evidenced by the asymmetry observed in the disk's outer regions. The galaxy's disk is viewed at an angle that is not quite edge-on but not face-on either. The disk and arm structures indicate that the galaxy is most likely a barred spiral galaxy.
