The galaxy presents a largely smooth, elliptical morphology. There is a high degree of central concentration of light, with the luminosity appearing to decrease radially outward. The core region exhibits a yellowish-white hue, suggesting the presence of an older stellar population. Fainter extended light with reddish hue is observed around the core. No distinct spiral arm structures or features are discernible in this image, which suggests the galaxy is relatively undisturbed. The galaxy's apparent roundness indicates a low degree of ellipticity and inclination with respect to the observer's line of sight. Given the smooth profile and color, it's likely an elliptical galaxy with a moderate stellar mass and a low star formation rate.
