The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. The light distribution is mostly uniform, exhibiting a high degree of symmetry. There is a slight elongation, but it is generally round. There are no discernible spiral arms or bar structures. The galaxy has an elliptical appearance with an overall yellow-white hue, suggesting an older stellar population. There is no obvious evidence of active star formation regions. No tidal tails or obvious signs of recent merger activity are present, though a small amount of disturbance cannot be ruled out at this resolution. 
