The galaxy presents a relatively smooth, elliptical morphology. It appears centrally concentrated with a bright, yellowish core, potentially indicating an older stellar population. The galaxy exhibits a degree of rotational symmetry. There's a subtle color gradient, transitioning from the yellower core to slightly bluer outer regions. This implies some ongoing, but moderate, star formation within the galaxy's extended disk. The overall structure suggests minimal disturbances, not exhibiting any signs of major mergers or tidal interactions. The galaxy is somewhat large and massive.
