The galaxy appears as a relatively smooth and concentrated object. It is generally elliptical in shape, exhibiting a high degree of roundness. The light distribution suggests a fairly uniform stellar population, without prominent spiral arms or distinct features like dust lanes. There is a notable lack of significant disturbances or signs of ongoing merger activity with other galaxies. The galaxy’s color exhibits a hint of blueness, implying that star formation is occurring. Overall, the galaxy appears to be a rather isolated system, with minimal external influence shaping its morphology.
