The galaxy presents an overall elliptical morphology. The central region exhibits a bright, concentrated core, indicative of a significant stellar population density, possibly a supermassive black hole. The color of the core is noticeably redder, suggesting an older stellar population dominated by red giant stars. The galaxy appears relatively smooth in texture, without prominent spiral arms or distinct features. The galaxy has a slight elongation, its shape is not perfectly circular, implying some degree of internal structure or a potential interaction with another galaxy. There's a subtle color gradient, with the outer regions of the galaxy appearing slightly bluer than the core, which could be due to the presence of younger stars or a small amount of ongoing star formation in the outer parts of the galaxy. Overall, the galaxy seems to be a relatively evolved system with a dominant spheroidal component.
