The galaxy appears as a single, centrally concentrated object with a smooth and relatively featureless morphology. It exhibits a near-spherical shape. There appears to be no evidence of spiral arms or a disk-like structure. The color profile shows a central region with a strong presence of light at green wavelengths, suggesting the presence of ionized gas, and/or a population of younger stars. The extended halo exhibits a more redshifted hue suggesting an older population of stars. The galaxy does not obviously display tidal tails or other major disturbances in its structure, although subtle signs of a minor disturbance or early-stage merger cannot be ruled out based on the image alone.
