The galaxy presents as an edge-on spiral, characterized by a prominent dust lane bisecting its central bulge. The bulge exhibits a smooth, rounded morphology with a yellow-orange hue, suggesting an older stellar population. The disk component appears thin and elongated, with subtle color gradients indicating regions of active star formation, particularly in the outer edges. A noticeable amount of dust is obscuring some of the light coming from the disk. The disk is slightly warped, and the galaxy does not seem to be undergoing any major mergers or violent processes.
