The galaxy presents a largely elliptical morphology, appearing quite smooth and relatively featureless. Its color profile suggests a dominant population of older stars, with a yellowish hue indicative of lower levels of on-going star formation. There is no strong evidence of spiral arms or a distinct galactic disk from this viewing angle, and it exhibits a concentrated central bulge. Minor disturbances cannot be ruled out, but it does not seem to be undergoing any major interactions or mergers. Overall, the galaxy gives the impression of being a mature system, possibly an elliptical galaxy which may be transitioning to, or has already reached, the red sequence.
