The galaxy presents a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated region, transitioning outwards to a less luminous and more diffuse halo. The shape appears moderately elongated, deviating slightly from a perfect sphere. There is a subtle suggestion of some irregularities, possibly minor disturbances within the galaxy, but this is not pronounced. The color profile indicates a generally older stellar population, with a yellowish hue in the central region, shifting to slightly bluer tones in the outer regions. There is little evidence of strong star formation within the galaxy.
