The galaxy presents as an edge-on spiral system. The disk appears elongated, with a notable central bulge. The bulge exhibits a smooth, rounded morphology. The overall color is indicative of an older stellar population, trending towards the redder end of the spectrum, particularly in the bulge. There's a slight indication of dust lane obscuration running along the midplane of the disk, though this is not strongly defined. There is no evidence of significant recent star formation, as evidenced by the absence of prominent blue regions or HII regions. The galaxy appears relatively undisturbed, showing no clear signs of ongoing or recent mergers or tidal interactions.
