The galaxy presents a primarily smooth morphology, with an elliptical-like shape appearing neither perfectly round nor highly elongated. It exhibits a dominant bulge component, indicated by the concentrated central brightness. There are hints of disk-like features, but they appear faint and not well-defined. The galaxy displays a yellow/orange hue, suggesting an older stellar population and minimal ongoing star formation. There is no clear evidence of any major mergers or significant tidal disturbances. The overall appearance suggests a relatively evolved system with a substantial stellar mass.