The galaxy presents a generally smooth, elliptical morphology. Its shape appears somewhat flattened, deviating slightly from a perfect sphere. The central region displays a high concentration of light, indicative of a substantial galactic nucleus. The galaxy exhibits a color gradient, appearing bluer in the inner regions, possibly signaling ongoing or recent star formation there. Fainter, redder hues in the outer regions suggest an older stellar population. There is a suggestion of possible minor disturbances in the form of subtle, elongated features. Overall, the galaxy seems to be an intermediate mass object with a low star formation rate.
