The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The overall color appears predominantly reddish-orange, possibly indicating an older stellar population. Some bluer regions are observed, more concentrated toward the outer regions of the galaxy. There are indications of minor disturbances in the morphology, possibly due to tidal interactions or a past merger event. The central region is notably smooth in appearance. Overall, the galaxy appears as a relatively massive system, exhibiting signs of ongoing, but not intense, star formation.
