The galaxy presents as a lenticular or edge-on spiral, exhibiting a disk-like structure with a noticeable central bulge. The bulge appears smooth and concentrated. The disk component is relatively faint and elongated, displaying a cigar shape. It is difficult to discern any distinct spiral arm structure. Overall, there is no substantial indication of active star formation. There is also little to no indication of mergers or tidal disturbances in the image.
