The galaxy presents as a somewhat elongated, lenticular structure with a noticeable central bulge. The galaxy's overall color is a yellowish-white hue, suggesting an older stellar population. The disk appears relatively smooth with a hint of possible spiral structure. The elongation suggests an elliptical morphology with a possible bar. There are no obvious signs of active star formation regions, such as HII regions or intense blue light. The central bulge appears brighter and more concentrated than the outer disk regions. There are no readily apparent signs of a major ongoing merger or tidal disruption, although a minor disturbance is not completely ruled out by the morphology.
