The galaxy appears to be a relatively smooth, elliptical type. Its central region exhibits a concentrated, bright core with a yellowish hue, suggesting an older stellar population. The light gradually diffuses outward from the core, transitioning into a less intensely colored halo. No distinct spiral arms or prominent dust lanes are visible. The galaxy's overall form suggests a high degree of sphericity. There is no obvious indication of a major ongoing merger event, though some subtle asymmetries in the outer halo warrant closer examination for minor disturbances.
