This galaxy appears as a centrally concentrated object, exhibiting a smooth morphology. The light distribution suggests a dominant spheroidal component. The core region displays a reddish hue, potentially indicating an older stellar population or dust obscuration. Surrounding the core, there's a slightly more extended, greenish halo. Given the absence of spiral arm structures or significant irregular features, this galaxy is likely an elliptical galaxy, possibly of moderate size and mass. There is no visible evidence of ongoing major mergers or significant tidal disturbances. The overall appearance suggests a relatively evolved system, with a low rate of star formation.
