The galaxy appears as a centrally concentrated system, exhibiting a smooth, elliptical morphology. A slight elongation is noticeable, suggesting a transition from a perfectly circular to a more cigar-shaped form. The color profile reveals a reddish core, likely indicative of an older stellar population dominating the central region. A subtle green hue surrounds the core, potentially indicating ongoing, but reduced, star formation in the outer regions. There are no prominent spiral arm structures or dust lanes visible, reinforcing the classification as a relatively undisturbed elliptical galaxy. There are only very minor signs of tidal disturbance or interaction with other galaxies in the area. The overall structure suggests a high level of morphological stability.
