The galaxy appears to be relatively compact and luminous. Its morphology is generally smooth and elliptical in shape, exhibiting a high degree of roundness. There are possible signs of interactions or tidal features, suggesting a past or ongoing merger event. Some disturbances in the light distribution can be seen, but overall the galaxy presents a primarily smooth, spheroid-dominated structure. The galaxy's color indices suggest an evolved stellar population, possibly indicating a low ongoing star formation rate.
