The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, suggesting a dominant bulge component. The color index indicates a redder spectral energy distribution. It is quite compact in apparent size, and its relative brightness suggests that this is a massive galaxy. The lack of visible spiral arms or distinct features points toward an older stellar population with a low star formation rate. There is no sign of ongoing mergers or tidal disturbances. It is largely a regular, undisturbed system.
