The galaxy presents as a relatively smooth, elliptical morphology. It appears moderately bright with a central concentration of light, suggesting a dense galactic nucleus. The color profile indicates a redder core transitioning to somewhat bluer outer regions, implying a potential mix of older stellar populations in the center and younger stars toward the periphery. There's a slight elongation, deviating from a perfectly circular shape. No prominent spiral arms or significant dust lanes are discernible in this image, however, there is a hint of a possible slight disturbance in the overall light distribution that may indicate it is a potential minor merger.
