The galaxy appears to be elliptical in shape, with a smooth, featureless morphology. There is no clear evidence of spiral arms or a distinct disk structure. The light profile suggests a centrally concentrated spheroid with decreasing intensity outward. The galaxy exhibits a color gradient, appearing more yellow/gold towards the center, likely indicating an older stellar population and a higher concentration of evolved stars in the core. The outer regions are slightly bluer, possibly indicating some ongoing, although low, levels of star formation in the galaxy's outskirts. There does not appear to be any significant signs of tidal disturbances or ongoing mergers, though a slight asymmetry in the outer halo could indicate a minor past interaction. The overall appearance points to a relatively quiescent and evolved system.
