The galaxy presents as a disk-shaped system, oriented approximately edge-on relative to our line of sight. A prominent central bulge is evident, exhibiting a yellowish hue suggesting an older stellar population. The disk component appears somewhat clumpy and displays a bluer color indicative of younger stars and ongoing star formation. There appears to be some asymmetry within the disk with one side of the disk displaying a broader and more diffuse structure. There are features suggesting minor disturbances in the outer regions.
