The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The color profile exhibits a redder hue, suggesting a dominant population of older stars. There is no indication of prominent spiral arms or a significant disk component. The galaxy appears relatively undisturbed, lacking any obvious signs of ongoing mergers or tidal interactions. The shape of the galaxy appears to be more elongated than perfectly circular, trending towards an elliptical shape. Overall, this object appears to be a typical elliptical galaxy at a considerable distance.
