This galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light profile. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the color transitions slightly to a redder tone, possibly indicating a difference in metallicity or age gradient within the galaxy's stellar populations. There is a subtle suggestion of a disk-like component but the smooth light profile indicates this is likely an elliptical galaxy. The overall morphology suggests minimal recent interactions or disturbances, although there may be some signs of minor disturbances on the periphery. The galaxy's red shift indicates that the light is stretched and the galaxy is travelling away from us.
