  In this work, we study the properties of galaxies that are showing the
inside-out assembly (which we call inside-out assembled galaxies; IOAGs), with
the main aim to understand better their properties and morphological
transformation. We analysed a sample of galaxies from the Sloan Digital Sky
Survey (SDSS) Data Release 8 (DR8), with stellar masses in the range $\log
M_{\star}=10.73-11.03$ $M_{\odot{}}$ at $z < 0.1$, and analyze their location
in the stellar mass-SFR and the color-stellar mass diagram. We found that IOAGs
have different spectroscopic properties, most of them being classified either
as AGN or composite. We found that the majority of our sources are located
below the main sequence of star formation in the SFR-stellar mass diagram, and
in the green valley or red sequence in the color-stellar mass diagram. We argue
that IOAGs seem to correspond to the transition area where the galaxies are
moving from star-forming to quiescent, and from the blue cloud to the red
sequence and/or to recently quenched galaxies.
