The galaxy appears as a relatively smooth, elliptical structure, approximately 11 kiloparsecs in radius. Its overall color is yellowish, suggesting a population of older stars. The galaxy appears to have a centrally concentrated, bright core, with decreasing luminosity towards the outer regions. There is a slight deviation from perfect circularity, tending towards an in-between shape. No prominent spiral arms or distinct disk-like structures are discernible, and there is no evidence of strong dust lanes or patchy star formation regions within this image. There may be a hint of minor disturbance in the system, as the structure is not completely uniform. There is no indication of a major merger event or tidal tails suggesting recent interaction with another galaxy.
