The galaxy presents as a relatively smooth object with a slightly elongated, but generally rounded morphology. It appears to be an early-type galaxy, likely elliptical or lenticular. The central region exhibits a higher surface brightness, suggesting a concentration of stars or a possible active galactic nucleus (AGN), though there's no clear indication of strong activity. The color gradient suggests a transition from a bluer inner region, potentially indicating younger stellar populations or ongoing star formation in the core, to a redder, more quiescent outer halo. There is no apparent presence of prominent spiral arms or a distinct disk structure. There are no clear indications of recent or ongoing major merger events. The overall structure is relatively undisturbed and smooth, suggesting that it is a relaxed system.
