This galaxy presents a primarily smooth, elliptical morphology. The galaxy is quite luminous. The shape appears roughly round, with a slight deviation towards an elongated form. There is a suggestion of a secondary nucleus or concentrated region of luminosity located near the primary galactic core. The colors observed suggest an older stellar population, with the redder components being more pronounced and possibly indicating lower levels of current star formation activity. Indications are that a merger is occuring with another galaxy.