The galaxy presents as an edge-on or highly inclined disk galaxy. A central bulge is visible, appearing prominent and somewhat concentrated. The dust lane is obscuring the plane of the disk with little to no signs of active star formation visible along the disk. The overall color of the galaxy appears reddish, consistent with an older stellar population. The lack of distinct spiral arm structures suggests the galaxy may be undergoing morphological transformation, or that active star formation is suppressed throughout the disk.