The galaxy presents as a lenticular or possibly spiral galaxy viewed edge-on or at a high inclination. The central bulge appears prominent, displaying a concentrated yellowish-white hue, suggestive of an older stellar population. A fainter, bluer disk extends outward from the bulge, indicating the presence of younger, hotter stars and potential ongoing star formation, however the color could be influenced by redshift. The disk's edges are somewhat ill-defined, fading gradually into the background sky. There is no apparent dust lane bisecting the galaxy, nor any distinct spiral arm structure visible in this image, which lends evidence it may be an edge-on lenticular galaxy. The overall form is relatively smooth and undisturbed, showing no obvious signs of recent major mergers or tidal interactions.
