The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with a high degree of roundness. The central region appears brighter and yellower compared to the outer regions, suggesting a concentration of older stellar populations in the core. There's a subtle color gradient extending outwards from the center, with a hint of bluer hues, implying the presence of younger stars or ongoing star formation activity in the galaxy's periphery. There is potentially a minor disturbance or asymmetry in the galaxy's morphology. Overall, the galaxy seems relatively undisturbed, with no prominent signs of major mergers or tidal interactions.
