The galaxy presents as an edge-on spiral or lenticular system. It exhibits a prominent central bulge, which appears relatively smooth and concentrated. The bulge displays a yellowish hue, potentially indicating an older stellar population. Extending outwards from the bulge is a flattened disk component. The disk appears thin and elongated, consistent with an edge-on orientation. The disk's color is generally bluer compared to the bulge, suggesting the presence of younger stars and ongoing star formation, though this appears minimal. There is no clear indication of distinct spiral arm structure, although some subtle variations in brightness within the disk may be present. Overall, the galaxy appears to be relatively undisturbed, without obvious signs of major mergers or tidal interactions.
