The galaxy presents a largely smooth and rounded morphology. Its color suggests a population of older stars, with a central concentration of light that fades gradually towards the outer regions. There is very little evidence of spiral arm structure or prominent dust lanes, which suggests it may be an elliptical galaxy or a lenticular galaxy viewed face-on. The light distribution appears largely symmetrical. There are no obvious signs of ongoing major merger activity or significant tidal disturbances. Any merging occurring would likely be a minor disturbance. 
