The galaxy presents a largely smooth, elliptical morphology. The light is concentrated towards the center, forming a bright, well-defined core that fades into the outskirts. The color of the core appears yellowish, potentially indicating an older stellar population. The outer regions of the galaxy show a slight blue tinge, which could be evidence of some on-going star formation, although limited. The overall shape is relatively round, lacking significant distortions that would suggest a recent or ongoing merger event. There is no apparent disk structure, and no obvious spiral arms.
