The galaxy presents a relatively smooth morphology, exhibiting characteristics consistent with an elliptical galaxy. The light distribution is concentrated toward the center, displaying a slight elongation. The color indices suggest the presence of an older stellar population. There is no evidence of ongoing, high intensity star formation within the galaxy. Some minor disturbances can be seen. There is no signs of merging with another galaxy. Overall, the galaxy appears to be a evolved system with a dominant spheroidal component.