The galaxy presents a smooth, elliptical morphology. Its color profile suggests a moderate age stellar population, with a yellowish hue indicating the presence of older, evolved stars and diminished star formation. The galaxy appears elongated, with an axial ratio suggesting a flattened ellipsoidal shape. There is no strong evidence of spiral arms or significant dust lanes. The light profile appears relatively uniform, lacking prominent central concentration or extended features. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There is a slight asymmetry in the galaxy's outer regions, potentially indicative of a minor interaction or internal processes. The overall structure suggests a relatively evolved galaxy that is slowly forming stars.
