The galaxy appears to be a relatively bright, elliptical-shaped object, exhibiting a smooth morphology with no discernible spiral arms or bar structure. Its color suggests a population of older stars, leaning towards redder wavelengths, potentially indicative of a lack of significant current star formation. The light is centrally concentrated, suggesting a dense core. There might be a very slight disturbance in its shape, but overall it appears to be an undisturbed galaxy.
