The galaxy presents as a relatively smooth, elongated object, likely a spiral galaxy viewed edge-on or a lenticular galaxy. There is little apparent substructure within the galaxy's light distribution. The central region is brighter and appears yellowish-orange, possibly indicating an older stellar population or the presence of dust obscuration. The galaxy's profile fades gradually towards the edges. There is no obvious evidence of a prominent disk, spiral arms, or recent major merger activity. The galaxy appears to be generally isolated, with no obvious signs of tidal interactions or ongoing mergers with neighboring objects. Its color indices suggest a moderate degree of star formation activity. The overall morphology points towards a galaxy with a significant spheroid component.
