The galaxy presents as an edge-on spiral, exhibiting a highly elongated morphology. A prominent central bulge is visible, appearing relatively smooth and rounded. The disk component of the galaxy is thin and extends outwards from the bulge, displaying a slight hint of structure with subtle variations in color and luminosity, although no distinct dust lanes are discernible. The overall color gradient suggests a possible active star-forming region present within the disk, but with the bulge appearing a more yellowed color. There is no apparent evidence of major interactions or mergers affecting the system. The general appearance is indicative of a well-defined but somewhat quiescent spiral structure.
