The galaxy presents an elliptical morphology, appearing predominantly smooth and featureless. Its central region exhibits a concentrated luminosity, transitioning into a more diffuse halo. There's a hint of a disk-like structure within the galaxy, but the smoothness indicates a relatively old stellar population and subdued star formation activity. The galaxy's shape is closer to an in-between shape on a roundness scale, with the galaxy appearing moderately elliptical, not perfectly spherical nor extremely elongated. The color gradient suggests a higher concentration of older, redder stars towards the center, with bluer tones potentially indicating younger stars in the outer regions. There is no obvious indication of major disturbances or a recent merger event in the galaxy's structure, though minor irregularities cannot be ruled out.
