This galaxy appears to be a relatively smooth, elliptical-like system, with a concentrated central bulge. The overall color profile suggests a population of older stars. The system's shape is generally elongated, but not highly so, trending toward a more rounded morphology. There is some evidence of a slight disturbance in the form of an off-center red colored region, implying potential interaction or internal activity of an unknown source. No distinct spiral arms or significant dust lanes are discernible in this image, and there are no obvious signs of a major ongoing merger. The galaxy appears to be relatively isolated.
