The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular in shape, displaying a high degree of rotational symmetry. The galaxy exhibits a color gradient, with a bright, yellowish core that transitions to a redder halo. No distinct spiral arms or bar structures are apparent. There are subtle variations in surface brightness, but overall the galaxy appears to be relatively homogenous in its stellar distribution. The light profile appears to be concentrated, with a rapid decrease in luminosity away from the galactic center. There are no signs of active star formation. This suggests that the galaxy is an evolved system with a relatively old stellar population. No tidal features or signs of recent mergers are visible, indicating that the galaxy has likely experienced a period of relative isolation.
