The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution suggests a relatively high degree of symmetry. The core region is noticeably brighter and exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, diffuse light extends outwards from the core, fading into the background. There is a subtle elongation along one axis, giving it a slightly flattened appearance, but it is generally round. There is no discernible spiral structure or prominent dust lanes. The overall color suggests a relatively quiescent system with low current star formation activity. There are no strong indications of any ongoing or recent major merger events, although minor disturbances cannot be ruled out.
