The galaxy presents as a single, relatively smooth object. It appears largely elliptical in shape, exhibiting a high degree of central concentration with no discernible spiral arms or a distinct disk structure. The color profile suggests an older stellar population, with light trending towards the redder end of the spectrum. There is a slight color gradient, with a more yellow or golden central region that is more compact, while a less compact region surrounds the core with a lighter color. There is no clear evidence of active star formation regions, such as HII regions or dust lanes. Overall, the galaxy seems to be a passively evolving system, undisturbed by recent major merger events, with only small disturbances. The galaxy's light profile suggests that the galaxy is well on its way to quiescence. 
