The galaxy presents a morphology consistent with an elliptical galaxy. The light distribution appears smooth and centrally concentrated, lacking prominent spiral arms or a well-defined disk. The galaxy exhibits an overall orange hue. There seems to be a second object with a similar hue nearby, suggesting a possible minor interaction with another galaxy or galactic remnant. There appears to be a low level of star formation as well as a high stellar mass. There may be ongoing merger activity. The galaxy is approximately 6.8 kpc across.
