The galaxy appears to be an elliptical galaxy with a smooth, relatively featureless morphology. It exhibits a concentrated central bulge that is yellowish-white in color, suggesting a population of older stars. The galaxy fades in intensity toward the edges, forming an extended halo of light. There appears to be little to no evidence of prominent spiral arms or significant dust lanes. The object is generally round in appearance. There are no immediately obvious signs of ongoing or recent major merger activity based on visible disturbances in its structure. Faint blue regions can be seen outside of the bright bulge, suggesting some possible star formation. 
