The galaxy presents as a relatively smooth, elliptical object with a prominent central bulge. The color profile suggests a strong red component in the core, transitioning to a slightly greener hue in the outer regions. This may indicate a population of older, redder stars concentrated in the galactic nucleus, with younger, star-forming regions contributing to the greenish tint at the periphery. The overall shape is leaning towards an in-between, slightly rounded, rather than perfectly spherical or elongated, morphology. There's no strong visual evidence of ongoing merging activity or significant tidal disturbances. The image shows no disk.
