The galaxy appears to be a relatively smooth, elliptical system. It exhibits a spheroidal morphology with a high degree of central concentration. The color gradient suggests a population of older stars, particularly in the central bulge. There's a noticeable lack of distinct spiral arm structures or significant dust lanes. The galaxy presents a slightly elongated shape, but is generally well-rounded. The overall light distribution indicates a mature stellar population with a low star formation rate. There are no obvious signs of recent major merger activity. 
