The galaxy appears as a singular, somewhat elliptical object, exhibiting a smooth, centralized concentration of light. There is a notable color gradient. The core region displays a yellowish-orange hue, suggesting an older stellar population or a concentration of dust. Moving outwards, the galaxy fades and slightly shifts to greener colorations, possibly indicating patches of younger stars or areas with different dust composition. The general form suggests minimal disturbance or ongoing merger activity. Its overall morphology seems consistent with an elliptical galaxy, showing a lack of distinct spiral arms or a well-defined disk structure. There is a hint of a subtle elongation.
