The galaxy presents as a relatively smooth, elliptical morphology with a dominant central bulge. The overall light distribution appears concentrated with a lack of spiral arm structure or distinct features. The color gradient suggests an older stellar population, with the central region exhibiting a yellowish-orange hue, transitioning to a bluer periphery. There is no obvious active galactic nucleus or significant dust lane obscuration visible in the image. The galaxy exhibits a high degree of roundness, showing no signs of major tidal disturbance or ongoing merger activity.
