The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The color profile suggests an older stellar population, with a dominant yellowish-orange hue throughout the galactic body. There is a subtle elongation observed, moving it away from being perfectly circular. No distinct spiral arms or prominent dust lanes are readily apparent. The outer regions of the galaxy fade gradually into the background sky, lacking sharp or well-defined edges. There are no indications of major ongoing merging events or significant tidal disturbances.
