The galaxy presents as a luminous, elliptical object with a high degree of central concentration. It exhibits a smooth, featureless morphology, lacking discernible spiral arms or a prominent disk structure. The color gradient suggests a population of older stars, contributing to the overall reddish hue. The galaxy is elongated, appearing more like a flattened spheroid than a perfect sphere. There is no obvious indication of a major ongoing merger, although there is a possibility of a minor disturbance. Based on this information, it can be inferred that the galaxy has a low star formation rate.
