The galaxy appears to be a relatively smooth, elliptical galaxy. It is characterized by a concentrated, bright central bulge, which gradually fades into a more diffuse halo. The galaxy exhibits a yellowish-white color, suggesting a population of older stars. There are no obvious spiral arms or dust lanes visible, reinforcing the classification of an elliptical galaxy. The shape is generally round, with only a slight elongation. There is no indication of any major ongoing merger events, but perhaps some indication of tidal disturbances.
