The galaxy presents as a relatively smooth and centrally concentrated object. It appears elliptical in shape, with a bright, diffuse core that fades gradually towards the outer regions. There is no strong evidence of a disk-like structure or spiral arms. The light distribution is fairly uniform, suggesting a lack of significant star formation regions or prominent dust lanes. Some slight color variations are visible, with a tendency toward redder hues in the central region, indicating a potentially older stellar population in the core. The outer regions exhibit bluer colors, possibly indicating more recent, but still modest, star formation activity there. There is slight indication of minor disturbances, but is not likely a major merger event. Overall, the galaxy appears to be a mature system with a significant spheroidal component.
