The galaxy appears to be an elliptical type, with a generally smooth and diffuse light distribution. It presents a somewhat rounded morphology, although not perfectly circular. The core region exhibits a higher luminosity, with colors trending toward the redder end of the spectrum. The overall shape is maintained as the luminosity diminishes towards the outer regions of the galaxy. There are no immediately obvious signs of spiral arms or a well-defined disk structure. Additionally, there is a small possibility of minor disturbance in the outer regions but they are not a highly noticeable feature of the galaxy.
