This galaxy presents as a relatively smooth, centrally concentrated object. It appears predominantly elliptical in shape, with no prominent spiral arms or a well-defined disk structure visible. There may be a very faint disk surrounding the central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths in the core, which may indicate a population of evolved stars and lower current star formation. A small amount of blue is visible, potentially indicating some areas of star formation. There is no visual indication of any major ongoing merger events or significant tidal disturbances. The overall morphology suggests a galaxy that has largely completed its major assembly and is potentially undergoing a period of quiescence.
