The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity gradient, suggesting a significant population of older stars. The galaxy appears to be fairly evolved. There are no apparent spiral arms or significant dust lanes that might indicate active star formation regions. The slight bluer color suggests that a small amount of star formation could be present. Overall, the galaxy displays a predominantly spheroidal shape with a subtle flattening, and only minor irregularities or disturbances are visible.
