The galaxy presents a morphology consistent with a spiral galaxy, though the spiral arms are not sharply defined. The galaxy exhibits a moderate-sized bulge region, with a yellow to orange hue, suggesting an older stellar population in the central region. The surrounding disk displays a bluer tint, implying ongoing or recent star formation. The disk appears somewhat flocculent, with less distinct spiral arm structures. There may be some minor disturbances or interactions influencing its shape. Overall, the galaxy appears as a somewhat disrupted spiral, exhibiting moderate star formation and a prominent, older bulge.
