The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a decreasing gradient of luminosity towards its outer regions. The galaxy appears to be undergoing a significant merger, with two distinct nuclei visible. Each core is bright and compact, suggesting a high concentration of stars in the galactic centers. There is no apparent spiral structure or dust lanes. The overall color is yellow, indicating an older stellar population with relatively little ongoing star formation. The lack of blue light suggests a paucity of young, massive stars. There are no visible tidal tails or other debris, but there is a general disturbed appearance about the object that suggests interaction. The shape is generally round.
