The galaxy presents as a largely smooth, elliptical-like structure. The core is a bright, concentrated yellow, suggesting an older stellar population with minimal active star formation. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major mergers. There are no visible spiral arms or prominent disk features. The light profile suggests a high degree of central concentration. A small amount of bluer emission is visible in the outer regions indicating that there may be a low level of recent or ongoing star formation at the edges of the galaxy. Overall, the galaxy appears as a massive, evolved system.
