The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. The light profile transitions smoothly from the bright core outwards, with a slight elongation discernible along its major axis, suggesting a deviation from a perfect spherical shape. The dominant color is a yellowish hue, indicative of an older stellar population. It exhibits a low star formation rate, as suggested by the lack of bright blue regions associated with young, massive stars. The overall morphology suggests a galaxy that has largely exhausted its gas supply, with star formation primarily concluded. A slight disturbance is visible to one side of the galaxy, indicating a potential past interaction or minor merger.