The galaxy presents a primarily smooth and elliptical morphology. A slight elongation is observed, but the overall shape is relatively uniform. The central region exhibits a concentration of light, suggesting a prominent galactic nucleus or bulge. The color profile transitions from a reddish hue in the core to a more greenish-blue coloration in the outer regions. This could indicate a radial gradient in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars distributed further out. There appears to be no distinct spiral arm structure or significant dust lanes visible in the image, reinforcing the smooth classification. Minor irregularities may be present in the outer regions, hinting at possible tidal interactions or past merger events, although the dominant feature is a relaxed, spheroid-like structure.
