The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a primarily elliptical morphology, though with some hints of a flattened disk-like structure. The light distribution appears predominantly smooth, with a gradual decline in brightness from the core outwards. The galaxy's color profile appears to have a slightly blueish hue. It has some minor distortions of the light, but on the whole appears to be an isolated system that has not undergone a major merger. We note that the system is likely undergoing a slower rate of star formation.