The galaxy presents as a single, centralized object. The core exhibits a smooth, concentrated light profile, appearing nearly circular. The galaxy displays a dominant spheroid component and lacks any obvious spiral arm structures, indicative of an elliptical morphology or a lenticular galaxy viewed face-on. The color gradient transitions smoothly from a yellow-white center to reddish hues in the outer regions. No significant signs of tidal disturbances or active galactic nuclei are discernible from the image. The galaxy appears to be relatively isolated, without any close companion galaxies or signs of on-going merger activity. The roundness of the galaxy indicates it is likely not highly inclined with respect to the line of sight. The light distribution suggests an evolved stellar population, with a gradual decline in star formation activity.
