The galaxy presents as a relatively smooth, elliptical or lenticular structure. A bright central bulge dominates the morphology, with the light intensity decreasing gradually outwards. There is a slight elongation, but overall the object appears close to circular in projection. The galaxy exhibits a color gradient, transitioning from a yellow-white core to a more reddish halo, suggesting older stellar populations are more dominant in the outer regions. There is no obvious disk component or spiral arm structure visible in this image. Additionally, there are no signs of significant tidal disturbances or ongoing major merger activity based on the observed morphology.
