This galaxy appears to be a relatively smooth, elliptical galaxy. It presents a concentrated central bulge that emits strongly in yellow wavelengths, indicating an older stellar population. The overall shape is generally round, showing little to no disk structure. A faint red plume emanates from the galaxy indicating possible tidal interaction or star formation. There are no obvious signs of major merging events but may be experiencing minor disturbances. The galaxy exhibits a considerable luminosity and mass, suggesting a large and evolved system with a low rate of star formation.
