The galaxy presents as a primarily smooth, elliptical structure. It exhibits a concentrated, bright central region, suggesting a dense stellar population. The color profile shifts from a yellowish core to a slightly greenish outer halo. The absence of distinct spiral arms or prominent dust lanes indicates that the galaxy is likely an early-type galaxy. There is only the slightest indication of any disturbance to its shape, suggesting it is likely not undergoing a major merger, but possibly some minor interactions are visible. The galaxy appears relatively isolated.
