The galaxy presents as an elliptical or lenticular-type system, displaying a generally smooth, featureless appearance. The light distribution suggests a concentration of older stellar populations towards the center, indicated by the yellowish-orange hue. The object's elongated morphology suggests it is not perfectly spherical, but rather somewhat cigar-shaped, with its longest axis being several times the length of its shortest. There is no discernible evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, showing no obvious signs of recent major merger events, or strong tidal disturbances. The object has a relatively high mass. The object has relatively low star formation. 
