The galaxy appears as a centrally concentrated object with a moderately bright core. A diffuse halo surrounds the central region, exhibiting a somewhat irregular shape. The color distribution suggests the presence of multiple stellar populations, with a bluer central region indicative of younger stars or active star formation, transitioning to a slightly redder halo which may suggest older, more evolved stars. There are hints of possible disturbances or tidal features in the outer regions, though the limited resolution makes it difficult to ascertain their nature conclusively. There may also be subtle indications of dust lanes or obscuration, but it is very difficult to tell from this image. Overall, the galaxy presents as a system undergoing some form of dynamical interaction or internal process causing morphological irregularities.
