The galaxy presents as a relatively compact and elliptical object. Its light is centrally concentrated, displaying a smooth and featureless morphology. The galaxy exhibits a diffuse blue-white hue, suggesting the presence of a moderate population of younger stars. There is no clear evidence of spiral arms or a prominent disk structure. The general appearance indicates a system that is not currently undergoing a major merger, though some minor disturbances may be present. It shows an intermediate ellipticity, leaning more towards a spheroidal shape than a highly elongated form.
