The galaxy presents as a single, relatively smooth, and centrally concentrated object. Its overall shape appears nearly circular. The light distribution suggests a bulge-dominated morphology. The color gradient transitions from a yellowish core to a redder outer region, possibly indicating an aging stellar population and reduced recent star formation activity within the bulge and an overall older population. There are no obvious signs of spiral arms or significant dust lanes. There appears to be no major interaction or disturbance.
