The galaxy presents as an elliptical morphology with a smooth, featureless appearance in the available image. There appears to be one primary, centrally concentrated bulge. The concentration of light is high in the core region, suggesting an older stellar population. The overall color is notably redder, which reinforces that the galaxy is likely comprised primarily of older stars with minimal current star formation. Based on the overall undisturbed morphology, major mergers are unlikely to have played a role in its recent evolution. There is a slight elongation in the shape, but it is mostly round. 
