The galaxy presents as a flattened, elliptical form, elongated along a major axis, with an approximate effective radius of 9 kpc. It exhibits a smooth morphological profile, characterized by a central bulge that appears yellowish. The outer regions of the galaxy show hints of a faint disk-like structure, with a bluer hue than the central bulge. The overall appearance is indicative of a galaxy undergoing low levels of star formation, or perhaps it is transitioning into a quiescent state. The galaxy does not show evidence of major merging activity, however there may be minor disturbances to its morphology. The galaxy is moderately large with an estimated stellar mass of roughly 10^11 solar masses.
