The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The primary light emission appears yellowish-orange, suggesting a population of older stars and a diminished rate of active star formation. There's a subtle elongation, hinting it's not perfectly spherical. The smooth texture suggests a well-mixed stellar population, consistent with an evolved system. Based on the estimated size, it is a medium sized galaxy. There is no evidence of major disturbances or ongoing mergers.
