The galaxy presents as an elliptical morphology, appearing largely smooth and featureless in the observed wavelengths. There is a clear color gradient, with a more concentrated yellowish-orange hue towards the galactic center, suggestive of an older stellar population and potentially a higher concentration of dust. The outer regions of the galaxy exhibit a fainter, bluer halo, which could indicate the presence of younger, though less prominent, star formation activity or a population of metal-poor stars. The galaxy is elongated, showing an "in between" round shape. No distinct spiral arms or bar structures are discernible. No evidence for any major ongoing merger events is observed. The overall appearance indicates a relatively evolved system.
