The galaxy presents an overall yellowish hue, indicative of a population of older stars. The central region is brighter and more concentrated, which could suggest a higher density of stars in the galactic nucleus, possibly surrounding a supermassive black hole. The shape of the galaxy appears somewhat irregular, showing some visible features and possibly minor disturbances. This suggests it may be undergoing or have undergone a galactic interaction or merger event, as the distribution of stars does not appear perfectly symmetrical. The morphology appears to be somewhere between a pure elliptical and a spiral galaxy. There may be ongoing star formation, but it seems to be at a relatively low rate.
