The galaxy presents an overall elliptical morphology, appearing somewhat flattened. There is a distinct central region displaying a brighter intensity. Surrounding this core is a more diffuse, extended halo of lower surface brightness. A subtle disclike structure may exist within the brighter central region. Features indicative of a major merger event appear to be absent. The image suggests a galaxy that is generally undisturbed, with no obvious tidal tails or other prominent signs of recent interaction. However, there may be a very minor disturbance present. The smoothness of the light distribution suggests that the galaxy is dominated by an older stellar population.
