This galaxy appears to be an edge-on spiral galaxy with a prominent central bulge. The dust lane is clearly visible bisecting the galaxy's light, indicating substantial dust obscuration within the disk. The disk itself appears thin and elongated, characteristic of a spiral galaxy viewed at a high inclination angle. The color profile suggests an older stellar population throughout the bulge and disk, with a general lack of bright blue star forming regions, although some star formation is present. The bulge seems to be centrally concentrated and shows no clear signs of a bar structure. The galaxy displays a relatively smooth morphology, showing no major disturbances or tidal features.
