This galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and featureless morphology. It has a somewhat elongated, but generally rounded shape, with the "in between" roundness being the highest round fraction. There are no distinct spiral arms or other readily discernible structures typically associated with disk galaxies. The galaxy displays a central concentration of light, suggesting a bulge component. The color is predominantly yellow-orange, which indicates an older stellar population with a low star formation rate. There is no apparent interaction with nearby galaxies or signs of a major merger event, though a minor disturbance cannot be ruled out.