This galaxy appears to be relatively compact and luminous. Its morphology seems smooth and elliptical, exhibiting a centrally concentrated light profile. The galaxy displays a color gradient, transitioning from blue-green hues on one side to a yellow-reddish hue on the other. This color variation may indicate differing stellar populations or dust content across the galaxy. There may be evidence of a minor interaction or disturbance present, as suggested by a slight asymmetry or a faint tidal feature. The overall structure doesn't show signs of a major ongoing merger. The size appears consistent with a galaxy of moderate scale, and its luminosity suggests a substantial stellar mass and star formation rate.
