The galaxy presents as a relatively smooth, elliptical-like structure, with a bright central nucleus. There is a slight elongation noticeable in the morphology. The radial light profile appears to decrease smoothly from the center outwards. The object exhibits a dominant spheroidal component with a notable absence of distinct spiral arms or significant dust lanes. The color is generally uniform, trending toward a slightly bluer hue. There is no visual evidence of any recent major merger events or strong tidal disturbances affecting the galaxy's morphology, though minor disturbances cannot be ruled out.
