The galaxy presents as a centrally concentrated, smooth object. Its morphology is generally elliptical, with a high degree of symmetry around the nucleus. There is a noticeable radial color gradient, transitioning from a brighter, slightly bluer center to a redder outer region. No distinct spiral arms or bar structures are visible, and no significant tidal disturbances or interactions with nearby galaxies are apparent. Based on its appearance, it most likely represents a relatively quiescent galaxy with a stellar mass nearing 10^11 solar masses, exhibiting low levels of ongoing star formation. The lack of prominent features points towards a more evolved system dominated by older stellar populations.
