The galaxy appears as a somewhat diffuse, centrally concentrated object. Its overall color is a pale blue, suggesting the presence of ongoing star formation. It has a relatively smooth appearance with some irregular regions, indicating possible disturbances or interactions. The shape is generally elliptical, but there are slight deviations from perfect symmetry. There is evidence of disk-like structure with some areas of organized star formation. There is no prominent central bulge visible, but a central concentration of light suggests an active region. Given its color and slight asymmetries, the galaxy appears to be actively evolving, although it is neither undergoing a major merger nor is it a classical spiral galaxy.
