The galaxy appears to be a relatively smooth, elliptical-like structure. Its core displays a concentrated luminosity, suggesting a significant stellar population in the central region. The light is dominated by redder wavelengths, indicating an older stellar population. Fainter blue regions on the edges suggests a small amount of star formation in the outer regions. There is a slight elongation to the galaxy’s shape, possibly indicating it may be an oblate spheroid. There are no readily apparent spiral arms or a prominent disk structure.
