The galaxy appears as a moderately bright, relatively smooth object. It exhibits a concentrated, rounded morphology. There is a slight elongation, but it appears largely spheroidal in shape. The color profile suggests a population of older stars, trending towards redder hues in the central region, with a slight bluer tinge in the outermost areas. There are no obvious spiral arms or a prominent disk structure. Indications of minor disturbances may be present, but the overall structure seems largely unperturbed.
