The galaxy appears to be an elliptical galaxy, with a smooth, featureless morphology. The central region displays a high concentration of light, which decreases gradually towards the outer edges. The light is mainly concentrated in the yellow and redder wavelengths, possibly indicating an older stellar population, meaning there are fewer new stars being born. There is no apparent spiral structure or dust lanes present. The overall shape is close to circular, though slightly elongated. There is no evidence of strong tidal features or ongoing major merging activity. The galaxy appears to be relatively isolated and undisturbed.
