The galaxy presents a roughly elliptical morphology, though some irregularities suggest possible disturbances or interactions. Its core region exhibits a high degree of central concentration with a yellowish hue, indicating an older stellar population. The outer regions fade in luminosity, displaying a bluer color, which is consistent with the presence of younger stars. There is a suggestion of a disk-like structure. The galaxy shows signs of possible minor mergers. There are some indications of ongoing star formation, evidenced by bluer regions of the galaxy. Overall, the galaxy appears as a fairly massive object.
