The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that diffuses outwards, with no apparent spiral arm structures. The overall color appears to be a pale yellow, indicative of an older stellar population, potentially with a low rate of ongoing star formation. There are no discernible dust lanes or regions of intense blue light indicative of recent, massive star formation. The galaxy appears largely undisturbed, with no obvious signs of a recent or ongoing merger event. Its profile suggests a high degree of rotational symmetry, conforming to a largely elliptical, spheroid shape.