The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, symmetrical structure with minimal discernible features. Its overall shape is notably round. The galaxy's light is concentrated toward the center, suggesting an older stellar population. There is some indication of a disk but it is not clear. The color appears to be largely homogenous with a slight yellow hue, implying a lack of ongoing star formation. There are no visible signs of recent mergers or major disturbances affecting the galaxy's overall form, though very minor disturbances cannot be ruled out.
