The galaxy appears to be an elliptical galaxy, exhibiting a smooth, rounded morphology with a high degree of central concentration. The light distribution suggests a relatively featureless structure, lacking prominent spiral arms or a well-defined disk. The galaxy displays a radial color gradient, with the core appearing more reddish-orange, transitioning to a bluer hue in the outer regions. This color gradient could indicate variations in stellar populations and star formation activity across the galaxy, with older, redder stars dominating the core and younger, bluer stars present in the outer regions. There is no evident distortion of the overall structure, and it appears that the galaxy is relatively isolated, showing no signs of recent major merger events or significant tidal interactions with nearby galaxies. Star formation is low.
