The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be elliptical. The color profile indicates a redder core with a slight blue tinge towards the outer regions of the galaxy. There is a noticeable lack of distinct spiral arm structures or features, suggesting a more evolved system. The galaxy appears to be isolated, with no obvious signs of ongoing major merger activity, although a slight asymmetry in the outer halo might suggest minor interactions or disturbances.
