The galaxy presents a generally smooth, elliptical morphology. It exhibits a pronounced central bulge, appearing as a concentrated region of luminosity. The light distribution around the bulge tapers off gradually. There is some subtle evidence of a disk-like structure, though it is not sharply defined. A small bright knot of light is also visible away from the center, and slightly offset from the central bulge. The color profile suggests a higher concentration of older stellar populations within the bulge, while the outer regions and knot exhibit bluer hues, indicative of more recent star formation activity. Overall, the galaxy appears relatively undisturbed.
