The galaxy presents a largely smooth, elliptical morphology. The galaxy's core exhibits a bright, concentrated luminosity, with a gradual decrease in surface brightness extending outward. The distribution of light suggests an older stellar population, with a dominant yellow-red hue. There is no obvious structure, such as spiral arms or a prominent disk component. The overall shape is close to round, with a slight elongation. There is no evidence of any major mergers or strong tidal disturbances.
