The galaxy presents a moderately bright, centrally concentrated morphology. The primary body of the galaxy appears largely smooth, with a roundish, but not perfectly circular, shape. There is a notable color gradient from the core outward, shifting from yellowish in the center to a slightly redder hue in the outer regions. There appears to be a distinct feature that is a redder object associated to the galaxy. There are no obvious spiral arm structures or significant dust lane features visible in the image. The galaxy does not appear to be strongly interacting, though the distinct redder area suggests a potential merging event or disturbance. The low star formation rate indicated from other values would be consistent with its apparent smooth structure and redder overall color, implying a population of older stars dominating the galaxy's stellar content. 
