The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominated by evolved stars. The isophotes appear to be nearly concentric and slightly elongated. There is no evident spiral arm structure or significant dust lane features. The color gradient shifts subtly toward redder hues in the outer regions, which could imply a change in the stellar population.
