The galaxy presents a relatively smooth morphology, lacking prominent spiral arms or a defined disk structure. It appears largely spheroidal in shape, exhibiting a high degree of central concentration. The core region displays a distinct reddish hue, possibly indicative of an older stellar population or significant dust obscuration. Moving outwards from the core, the galaxy transitions to a more greenish-yellow color profile suggesting younger stars or the absence of dust. The outer regions of the galaxy gradually fade into the background, exhibiting a smooth, almost featureless profile, with no indications of major tidal disturbances or ongoing mergers. Overall, it seems to be an evolved galaxy with a fairly old stellar population.
