This galaxy presents as an edge-on spiral, or possibly a lenticular galaxy, exhibiting a prominent central bulge. The bulge appears roughly spherical and concentrated, showing a smooth light distribution suggestive of an older stellar population. There is a disk component that extends above and below the bulge. The color is predominantly reddish/orange in the central regions, indicative of older stars and possibly dust obscuration. The overall structure is elongated, typical of an edge-on view, and displays no significant signs of ongoing merger activity or major disturbances. Some dust and gas might be present in the disc of the galaxy. The galaxy appears to be fairly isolated, without any nearby companion galaxies that might influence its morphology.
