The galaxy presents as a relatively smooth and rounded structure, with a concentration of light towards the center. The light distribution suggests an elliptical morphology, lacking prominent spiral arms or a well-defined disk. A slight elongation can be observed, but overall the shape is close to circular. The color appears yellowish-orange, possibly indicative of an older stellar population. The absence of distinct blue regions suggests that active star formation is not dominant. There are no signs of major disturbances or merger activity within the galaxy's structure.
