The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape appears nearly circular, with a slight elongation evident. The light distribution suggests a dominant spheroidal component. There is no prominent spiral arm structure or obvious disk features visible in this image. The galaxy exhibits a color gradient, with a bluer central region and a redder halo. There is no evidence of a major ongoing merger or significant tidal disturbance. Some faint features may indicate a minor interaction with another object, or perhaps some very faint star formation is happening at the very edges of the galaxy.