The galaxy appears as a single, concentrated luminous object. It exhibits a smooth, symmetrical morphology with a predominantly elliptical shape. The core region presents a bright, relatively uniform intensity. The galaxy's color profile suggests a mature stellar population, exhibiting a yellowish hue overall. There are no immediately apparent features indicative of spiral arms or a prominent disk structure. No significant dust lanes or signs of active star formation are visually discernible. There might be very minor indications of asymmetry or subtle disturbances in the outer regions, but it mainly presents as a relaxed system with no major ongoing merger events. It exhibits a compact appearance, suggesting a relatively high stellar density within its observed volume.
