The galaxy presents a flattened, elliptical morphology. It exhibits a smooth, concentrated central bulge, indicative of an older stellar population. The light distribution suggests a relatively uniform structure without prominent spiral arms or distinct features. The galaxy's color is predominantly yellow-orange, implying a lack of significant ongoing star formation and a dominance of older, redder stars. There's no apparent dust lane or active galactic nucleus activity visible in this image. The galaxy appears relatively undisturbed, showing no signs of recent major mergers or significant tidal interactions. Its elongated shape suggests it may be an elliptical galaxy viewed from an angle or a lenticular galaxy with a weak disk component.
