The galaxy appears as a single, dominant, elliptical structure with a smooth, featureless morphology. It presents a spheroidal shape, exhibiting a high degree of roundness. There is no apparent disk or spiral arm structure. The galaxy's light is concentrated towards the center, with a gradual decrease in intensity outwards. Color gradients are subtle, with a slightly redder hue in the central regions, suggesting an older stellar population. There are no indications of ongoing major mergers or significant tidal disturbances affecting its structure. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
