The galaxy presents as a relatively smooth elliptical structure, displaying a noticeable elongation along its major axis. The core region exhibits a higher concentration of light, appearing more red-shifted in color. Moving outwards from the center, the light gradually diffuses, and the overall color shifts towards the blue end of the spectrum. There are no prominent spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. The galaxy appears to be a relatively quiescent system, with little evidence of recent or ongoing merger activity. The galaxy possesses a well-defined boundary. The overall morphology suggests a galaxy that has largely exhausted its supply of gas and dust, with stellar populations dominated by older, redder stars.
