The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The light distribution appears close to circularly symmetric, indicating a low degree of ellipticity. A color gradient is observed, with a yellowish core gradually transitioning into a greenish hue towards the outer regions of the galaxy. The overall color suggests an older stellar population dominates, although there might be some ongoing star formation. There is no apparent sign of tidal disturbances or merging activity, nor do there appear to be any notable spiral arms or a prominent disk structure. The galaxy's luminosity profile seems to decrease smoothly from the center outwards, lacking distinct breaks or rings.
