The galaxy appears as an elliptical structure, displaying a smooth, relatively featureless morphology. The light distribution exhibits a strong central concentration, gradually fading towards the outer regions. Color gradients are subtle, with a generally redder hue toward the core, suggesting an older stellar population. There may be a very slight indication of a disturbed morphology in the galaxy's outer regions, and a possible interaction. The galaxy is moderately large in extent, with an intermediate axial ratio, appearing neither perfectly circular nor significantly elongated. 
