The galaxy presents as a flattened, disk-shaped structure, viewed nearly edge-on from our line of sight. A prominent central bulge is visible, exhibiting a smooth, concentrated distribution of light that gradually decreases in intensity outwards. The bulge appears more yellow/orange in color, indicative of an older stellar population. The disk component exhibits a bluer hue, suggesting the presence of younger stars and ongoing star formation. The disk material is asymmetrical, with one side appearing extended in comparison to the other. There is a lack of defined spiral arm structures, and the edges are not well defined. It does not exhibit any signs of major disturbances or interaction with another galaxy.
