The galaxy presents an elliptical morphology, with a bright, concentrated central region. The core exhibits a cyan color, suggesting potential emission from ionized gases.

Moving outward, a diffuse, greenish halo surrounds the core. The green hue indicates the presence of star formation activity or [O III] emission, though its origin would require spectroscopic confirmation. The outskirts of the galaxy appear more irregular. There is evidence of possible tidal disturbances. There is a potential sign of minor interaction or merging event in the galaxy's shape. Faint, extended plumes are visible in the image.

Overall, the galaxy shows characteristics of both an elliptical galaxy, with its smooth central bulge, and a potentially disturbed system, as indicated by the outer, irregular features.
