The galaxy appears as a centrally concentrated object exhibiting a smooth, elliptical morphology. It is observed to have a yellow hue, indicating a potentially older stellar population. A slight elongation is visible; however, the overall structure is dominated by a near-spherical component. There is no observable presence of spiral arms, distinct dust lanes, or any irregular features typically associated with active star formation regions or ongoing mergers. Minor asymmetry is seen in the halo. It appears relatively isolated, showing no signs of major tidal interactions or recent merger events. Overall, the galaxy displays characteristics consistent with a mature elliptical system.