The galaxy appears as a centrally concentrated, diffuse object. It exhibits a smooth, elliptical morphology with no discernible spiral arm structure. The overall color is yellowish-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no prominent dust lane or evidence of significant obscuration. The light distribution appears quite uniform throughout the galaxy, further supporting the smooth classification. There are no obvious signs of tidal interactions or major disturbances.