The galaxy presents as a centrally concentrated object, likely an elliptical or early-type spiral, showing a smooth, relatively featureless morphology. It appears largely spheroidal in shape, with a high degree of circularity. There is no evident disk component or spiral arm structure. Faint disturbances are not apparent in the image, which indicates no major mergers or disturbances in its recent history. The galaxy exhibits a reddish hue, indicating that the stellar population is evolved with reduced star formation. The estimated size suggests that it is a fairly massive object.