This galaxy presents as a relatively compact object, with a smooth, elliptical morphology predominating. There is a subtle disk-like structure surrounding the central bulge, though it appears largely featureless. The overall color suggests a population of older stars, possibly with ongoing, but relatively subdued, star formation. There is no strong indication of a recent major merger event, though a minor disturbance or tidal feature cannot be entirely ruled out based on the image alone. The apparent roundness of the galaxy suggests a classification leaning towards E0-E3 on the Hubble sequence.
