The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge, which appears to be a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, with a bluer tint hinting at the presence of younger stars in its spiral arms or disk. There is no obvious evidence of strong tidal features, major mergers, or significant star formation. The lack of irregular structures suggests a relatively undisturbed evolutionary history. However, there is a minor amount of blue, which could indicate some recent star formation, or it is simply the color shift from distance. The shape is generally round with slight ellipticity.