The galaxy appears to be a relatively smooth, elliptical system. It presents a concentrated central bulge that gradually diffuses outward, lacking any distinct spiral arm structures or features. The overall color profile suggests a population of older stars, leaning towards a redder hue, indicative of lower rates of current star formation. The morphology appears largely undisturbed, with no prominent signs of tidal interactions or recent mergers. The galaxy's shape is nearly circular, suggesting a relatively low rotational velocity. There may be a supermassive black hole at its center.
