This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, suggesting a dense concentration of stars. The light profile appears centrally concentrated, decreasing in intensity with radial distance from the core. There is a slight elongation visible, deviating from a perfectly circular morphology. No prominent spiral arm structures or significant dust lanes are discernible. Overall, the galaxy appears to be a relatively undisturbed system with a well-defined structure. The color indices suggest a more evolved stellar population with a lower ongoing star formation rate. There is no obvious indication of a major ongoing merger event, although subtle signs of minor gravitational disturbances cannot be entirely ruled out based on this image alone.
