The galaxy presents as a single, relatively smooth, and well-defined object. It is elliptical in shape with a high degree of circularity. The galaxy exhibits a concentrated central bulge that gradually diffuses into a less dense halo. The color profile displays a yellowish core region, suggesting an older stellar population. There may be faint disturbances or minor irregularities in the outer halo, but they are subtle. The galaxy does not appear to be undergoing any major merger activity, but there is a slight asymmetry to its shape which may indicate a small disturbance.
