The galaxy presents as a relatively smooth, disk-like structure, viewed at a significant inclination. A central bulge region is visible, appearing somewhat brighter and more concentrated than the surrounding disk. The color of the central bulge seems slightly redder compared to the rest of the galaxy. The disk itself exhibits subtle color variations, with hints of bluer regions possibly indicating areas of star formation. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of a major merger. There are some slight irregularities in the disk and it is not perfectly smooth, indicating minor disturbances or ongoing interactions. 
