This galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology suggests a spheroidal shape, with a high degree of central concentration. There is no evidence of significant disk-like features or spiral arms. The color profile indicates a predominantly older stellar population, with a yellowish-orange hue suggesting a lack of ongoing, significant star formation. There may be indications of a minor disturbance or perhaps a recent minor merger event, though this is uncertain. Overall, the galaxy appears to be a passively evolving system.
