The observed galaxy presents as a relatively smooth, rounded structure. The primary color appears to be a yellowish-orange hue, concentrated centrally, with a slight color gradient outwards that becomes slightly bluer. There is no prominent disk-like structure or spiral arm features visible. There are no obvious signs of any major ongoing merging events or significant tidal disturbances, although minor irregularities cannot be ruled out based on the image alone. The overall morphology suggests a spheroid-dominated system, with the potential for a small amount of on-going star formation. The high degree of roundness reinforces the possibility that it is elliptical in shape.
