The galaxy presents as an elliptical morphology, with a smooth, concentrated light distribution. The color profile indicates an older stellar population, showing a significant red-yellow hue concentrated towards the center. There are no apparent spiral arms or dust lanes visible in this image, and the overall structure suggests a relatively evolved system, likely exhibiting very low rates of on-going star formation. The galaxy appears relatively undisturbed, without any signs of major mergers or tidal distortions. The isophotes suggest an intermediate ellipticity.
