The galaxy appears as an elliptical, elongated structure with a smooth morphology. Its central region exhibits a concentrated, bright core, likely indicative of a bulge. The color gradient suggests an older stellar population dominating the core, with the light shifting towards redder wavelengths. The outer regions of the galaxy show a bluer hue, potentially indicating the presence of younger stars or ongoing, albeit subdued, star formation. The overall lack of distinct spiral arms or irregular features suggests a quiescent galaxy, possibly in a later stage of its evolution. There is a very slight hint of a disk-like structure, but it is not well-defined. No significant signs of tidal disturbances or recent mergers are visually apparent.
