The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a smooth, rounded morphology. The disk appears thin and elongated, with the majority of the disk appearing to be at the same relative declination. There is a slight suggestion of a boxy bulge. The color of the bulge appears to be redder than the disk, potentially indicating an older stellar population. The disk shows a gradient in color, with the outer regions appearing more bluish, suggestive of ongoing star formation. There are no obvious signs of strong tidal interactions or major mergers. The galaxy appears relatively undisturbed.
