The galaxy appears to be an elliptical morphology, with a high degree of central concentration. It exhibits a smooth, featureless light distribution. The color profile suggests an older stellar population, with a reddish-yellow hue dominating the central region. There is no discernible spiral arm structure or dust lane features. The overall shape is close to round. There is no evidence of a major ongoing merger, although there could be minor disturbances visible. The light is somewhat extended.
