The galaxy presents as a centrally concentrated, relatively smooth object. The light profile appears to gradually decrease in intensity moving outward from the core. There's no clear indication of spiral arms or a distinct disk structure. The overall shape tends toward round, though with a slight deviation. There may be a hint of faint, disturbed tidal features extending from the galaxy's main body, suggesting a past or ongoing interaction. Colors range from yellowish-orange in the core to greenish-blue in the outer regions, possibly indicating varying stellar populations or dust content throughout the galaxy. The galaxy does not appear to be undergoing major merger activity.
