The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated luminosity, suggesting a significant density of stars. The radial light profile appears to gradually decrease from the center outwards, lacking any distinct features such as spiral arms or a prominent disk. The overall color appears to be slightly redder. The smooth morphology, concentrated core, and redder color index may suggest a more evolved stellar population with less ongoing star formation. There may be minor disturbances. There isn't any evidence of a significant merger.
