The galaxy presents as a relatively smooth and elliptical structure. The central region exhibits a bright, concentrated core that gradually diffuses outwards into a more extended halo. There is a distinct color gradient visible, with the core showing a bluer hue that transitions to a redder color in the outer regions. The overall shape suggests a disk, but without any pronounced spiral arm structures. There appears to be a slight elongation, indicating it is not perfectly circular but somewhat oval in shape. No significant tidal disturbances or merging features are immediately apparent. The overall morphology points towards a relatively evolved galaxy that may be undergoing moderate star formation activity.
