Observed galaxy exhibits a prominent spiral structure. The galaxy is not perfectly face-on, but presented at a slight inclination. The spiral arms are well-defined and appear tightly wound around the central bulge. A strong central bar is visible, bisecting the core region. The bulge itself appears moderate in size compared to the overall galaxy disk. Two spiral arms are most prominent. There are indications of ongoing star formation, as evidenced by the blueish hue of the arms and the clumpy structures within them. The galaxy is generally well-defined with no obvious signs of a major merger, although minor disturbances may be present.
