The galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth and concentrated light distribution. The overall shape is generally round, with no discernible spiral arm structure or a prominent bar. It possesses a dominant central bulge. There are indications of past or ongoing interactions, perhaps a merger of several galaxies, which have disrupted its original form, with three distinct bright regions that could be the galactic cores of each galaxy. There is an estimated redshift of approximately 0.103, placing the galaxy at a considerable distance. The galaxy exhibits a range of stellar populations, as indicated by variations in color across the image. Specifically, the central bulge appears to have a yellow/orange hue, indicating an older population of stars, whereas a fainter region of blueish light near the center may indicate younger stars.
