The galaxy presents as a centrally concentrated object with a smooth light distribution. The morphology appears to be elliptical, showing no spiral arm structure or distinct disk-like features. The galaxy displays a yellowish hue, indicative of an older stellar population with relatively low ongoing star formation. It is generally round in shape with a hint of elongation. There are no signs of any recent major merging activity, though some minor asymmetry or subtle disturbance within the galaxy's outer regions cannot be entirely ruled out given the resolution of the image.
