The galaxy presents as a moderately bright object with an apparent elliptical morphology. The central region exhibits a high surface brightness, appearing nearly uniform in color, predominantly blue, suggestive of a population of hot, young stars. The outer regions show a gradual decrease in surface brightness. Evidence of some low-level asymmetry is suggested by the slight distortions in the light distribution, particularly toward the northern edge. The slight disturbances potentially indicate an ongoing or recent gravitational interaction. There is a slight color gradient from blue at the center to redder hues in the outskirts, possibly indicative of older stellar populations in the galaxy's halo. The overall appearance suggests a system with a central bulge and hints of a disk, though the structure is not clearly defined.
