The galaxy appears as an elliptical-like structure with a smooth, centrally concentrated light distribution. Its shape is elongated. The galaxy exhibits a bright core, which gradually diminishes in intensity toward the outer regions. There is some hint of a disk galaxy due to it's apparent flatness, but any definitive spiral structures are absent. The color profile suggests a predominantly older stellar population, with a general absence of bright, young, blue stars. The presence of dust lanes or other forms of interstellar matter is not readily apparent. The overall morphology indicates that this system is at least fairly settled, without evidence of major ongoing mergers or significant tidal disturbances.
