The galaxy appears as a relatively bright, concentrated object with a smooth, elliptical morphology. The light distribution suggests a high degree of central concentration, with a gradual fall-off in luminosity towards the edges. The galaxy's color is primarily yellowish-red, suggesting an older stellar population and a possible lack of ongoing, significant star formation. There is no discernible spiral structure or obvious dust lanes visible in this image, reinforcing the impression of an elliptical type galaxy with a substantial mass. The overall impression is that of a well-formed, relatively undisturbed galaxy that is not undergoing active merging or significant tidal interactions. It presents as a mature system, dominated by older stars with minimal ongoing star formation.
