The galaxy presents as a somewhat elliptical, extended structure. The core region exhibits a high degree of luminosity, suggesting a concentration of stellar mass. This central bulge appears smooth and featureless, transitioning into a more diffuse halo region. There appears to be only a slight disk. The galaxy exhibits a yellow/orange hue, potentially indicative of an older stellar population. There appear to be some possible minor disturbances/indications of a potential merger, but it is difficult to confirm based on the image.
