This galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a yellowish hue, possibly indicating an older stellar population or significant dust obscuration. Moving outwards from the core, there is a faint greenish-blue halo surrounding the central region. This color suggests the presence of younger, hotter stars and ongoing star formation. The galaxy appears largely undisturbed, with no obvious signs of tidal tails or major mergers. There is a slight irregularity in the outer isophotes, but they remain generally elliptical in shape. Overall, this galaxy appears to be a relatively quiescent system with a mix of stellar populations, with its brightest magnitude being in the g band.
