The galaxy presents a concentrated, elliptical morphology. The light distribution is dominated by a smooth, centrally concentrated bulge, indicating a high degree of spheroidal symmetry. The galaxy appears to have some degree of disturbance, possibly a minor interaction. There is a hint of a disk, but if so it is small and nearly edge on. The galaxy's color gradient suggests an aging stellar population, particularly in the bulge, where the light is redder. The colors of the galaxy also point to a small amount of current star formation.
