The galaxy presents as a relatively smooth, concentrated object, likely an elliptical or lenticular galaxy. It exhibits an overall yellowish-orange hue, suggesting a population of older stars and a lower rate of active star formation. There is a hint of asymmetry, possibly due to a minor gravitational disturbance, but the overall structure lacks prominent spiral arms or a distinct disk component. The galaxy's light profile appears relatively compact, with a moderately high degree of central concentration. The object seems somewhat round, verging on being in between round and elliptical in shape. This galaxy does not appear to be undergoing a major merger, but might have a minor disturbance.