The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It presents a generally round morphology, with only a slight deviation from perfect circularity. The color profile suggests a population of older stars, given the yellow-orange hue, with little evidence of ongoing significant star formation. There is a subtle color gradient from the center outwards, with the core appearing slightly brighter and more yellow. There is little evidence of spiral arms or dust lanes, supporting the classification as an elliptical. Overall, the galaxy gives the impression of a mature system that has largely exhausted its gas supply for star formation.
