The galaxy appears as a relatively smooth, elliptical-like structure. It presents a concentrated central bulge which emits light more intensely than the outer regions of the galaxy. The central region of the galaxy appears yellow to golden in color, becoming more diffuse and slightly redder toward the outer edges. There's no indication of spiral arms or a well-defined disk in this particular observation. Faint color variations across the main body of the galaxy might suggest some differences in stellar population, though the overall homogeneity of the light indicates a well-mixed system. There is no apparent strong dust lane or any pronounced feature indicating a recent major merger event. There may be a slight asymmetry in the distribution of light toward the periphery, potentially suggesting a past interaction or minor disturbance.
