The galaxy presents as an elliptical morphology, appearing relatively smooth and concentrated. There is a yellowish central region, possibly indicative of an older stellar population. The outer regions exhibit a slight bluish hue, which might suggest the presence of some younger, hotter stars, though the extent of any star formation appears limited. The galaxy does not show any distinct spiral arm structure or a prominent disk. There is also no obvious evidence of an ongoing major merger, though subtle asymmetries or disturbances cannot be entirely ruled out based on this image.