The galaxy presents as a slightly inclined disk galaxy, exhibiting a notable bulge component that appears to be a dominant feature. The bulge displays a smooth, yellowish-orange hue, suggesting an older stellar population and relatively low levels of ongoing star formation within this central region. The disk itself shows evidence of some structure, with subtle variations in brightness and color, indicative of spiral arm segments. These arms appear somewhat flocculent and loosely wound. Blueish regions of the disk are suggestive of recent or current star formation. Overall, the galaxy appears to be undergoing some form of disturbance, as evidenced by the asymmetrical distribution of light within the disk, possibly indicating a weak gravitational interaction. The dust lanes within the disk are not easily discernible.
