The galaxy presents a relatively smooth, elliptical morphology with a noticeable central bulge. The galaxy displays a color gradient, transitioning from a bluer hue in the outer regions to a more reddish-yellow core. This suggests the presence of older stellar populations concentrated towards the center. The absence of well-defined spiral arms and the overall smoothness of the light distribution indicate the galaxy is likely an early-type galaxy. There are no clear signs of significant dust lanes or prominent star-forming regions. The lack of obvious tidal features or distortions suggests it has not undergone a major merger event recently, though there may be very minor asymmetries.
