The galaxy appears to be a luminous, elliptical system. It presents a smooth, featureless morphology, with a high degree of central concentration. The light profile suggests a fairly homogenous stellar population, lacking the distinct spiral arm structures characteristic of disk galaxies. The galaxy appears round, rather than elongated. There are no obvious signs of recent major merger events, though minor disturbances cannot be ruled out at this resolution. The system exhibits a color gradient, with a slightly redder core region transitioning to a bluer outer halo. The object seems relatively isolated in its immediate environment.
