The galaxy presents a smooth, elliptical morphology with a slightly elongated profile. The central region displays a concentrated luminosity, appearing nearly spherical. A color gradient is observed, transitioning from a yellowish core to a redder halo. There is a lack of discernible spiral arms or distinct dust lanes. Marginal irregularities may indicate minor gravitational interaction with another galaxy, but the overall structure suggests it is not undergoing a major merger. The galaxy is relatively compact, suggesting it is at intermediate distance.
