The galaxy appears as a relatively smooth, elliptical-like structure. It presents with a concentrated central bulge, bright and yellowish in color, suggesting a population of older stars. There is a faint extended halo surrounding the central region. No distinct spiral arms or dust lanes are discernible in this image. The galaxy appears to be quite round in shape, showing no strong elongation or distortion, suggesting it is not currently undergoing a major merger event. The overall light distribution appears relatively uniform, with no obvious signs of significant star formation regions.
