This galaxy exhibits an elliptical morphology, appearing generally smooth and somewhat elongated. The color gradient suggests a higher concentration of older stellar populations towards the galactic center, which displays a pronounced yellowish-orange hue. Fainter, bluer regions extend outward from the center, implying the presence of younger stars. The lack of strong spiral arm structures or significant dust lanes further supports the elliptical classification. There is some visual indication of a minor disturbance in the outer regions of the galaxy.
