The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is approximately circular. There is a distinct color gradient, transitioning from a reddish central core to a greenish outer halo. The red core suggests an older stellar population, whereas the green halo could indicate ongoing star formation, although the red and green colors in the images are also determined by the filter in question. This outer region is faint and appears diffuse. No spiral arm structures or significant dust lanes are discernible. There may be some slight tidal disturbances or minor indications of interaction, but if this galaxy is experiencing a merger, it is in its late stages. 
