The galaxy presents a mostly smooth, elliptical morphology with a high degree of roundness in its overall shape. It exhibits a concentrated central bulge with light that fades outwards. There are no spiral arm structures or prominent dust lanes visible. There are no signs of major disturbances or tidal features to indicate ongoing or recent major merger activity. There is some asymmetry in the halo or outer regions of the galaxy suggesting that there has been a minor gravitational interaction with another object in the past. The light distribution appears fairly uniform and consistent with a population of older stars. The galaxy exhibits a reddish hue.