The galaxy presents a largely smooth, elliptical morphology. Its light is concentrated in the center, fading gradually outwards. The central region exhibits a yellow-white hue, suggesting a population of older stars. The outer regions of the galaxy have a hint of blue-green coloration, which may indicate pockets of younger stars or some ongoing star formation. There is no clearly defined disk structure or spiral arms visible. No obvious signs of tidal disturbances or ongoing major mergers with other galaxies are apparent. The galaxy exhibits a relatively uniform appearance, and has an estimated radius of approximately 5 kpc.
