This galaxy presents as an elliptical-type galaxy with a smooth, concentrated light profile. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, the galaxy displays a subtle color gradient, transitioning to a greenish tint. This gradient could be indicative of ongoing star formation. The galaxy appears somewhat elongated, but generally round. There is no evidence of major mergers or tidal disturbances from this view. The overall morphology points towards a relatively evolved system experiencing modest levels of star formation.
