The galaxy appears as a concentrated, luminous object with a generally smooth, elliptical morphology. Its light profile suggests a centrally concentrated bulge, with a gradual decrease in intensity towards its outer edges. No distinct spiral arm structures or dust lanes are discernible in this image, implying a lack of significant ongoing star formation in a disk. The overall color seems relatively uniform, hinting at a population of older stars. There is no strong evidence of tidal features or morphological distortions, suggesting it is not currently undergoing a major merger event. It exhibits a round shape, neither highly flattened nor significantly elongated.
