This galaxy presents a largely elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. The core region displays a bright yellowish hue, suggesting an older stellar population dominating the galactic center. Moving outwards from the core, the color transitions subtly to a redder tone within the galaxy's halo, indicative of a progression to potentially older stars or a higher metallicity. There is little evidence of spiral arm structures or prominent dust lanes. The overall appearance suggests a system that is either a spheroidal galaxy or an elliptical galaxy viewed along its major axis, with no immediate signs of ongoing major merger events or significant tidal disturbances. A high level of central light concentration, and absence of blue light, suggests low levels of star formation throughout this system.
