The galaxy presents as an elliptical structure with a smooth, centrally concentrated luminosity profile. It appears to have a slightly elongated shape. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. The outer regions display a subtle color gradient, transitioning to a bluer tint, possibly indicating the presence of younger stars or a small amount of on-going star formation in the outskirts. There are no discernible spiral arms or distinct dust lanes. The overall morphology suggests a relatively evolved system with limited recent major merger activity. Minor irregularities are subtly present, hinting at the possibility of minor interactions or internal disturbances.
