The galaxy presents as a relatively compact object with a smooth, featureless morphology. Its shape is somewhere between elliptical and disk-like. The light distribution appears centrally concentrated, with a gradual decline in surface brightness outward. The galaxy has a yellow-orange hue, suggesting a population of older stars. There is a faint hint of an extended structure. There are no strong signs of ongoing star formation or active galactic nuclei activity visible. There does not appear to be any major ongoing mergers but the galaxy exhibits a minor disturbance in its shape.
