The galaxy presents as an elliptical morphology. It appears largely smooth and centrally concentrated, with a gradual decrease in surface brightness from the core outward. The galaxy exhibits a moderate color gradient, transitioning from a relatively redder core region to a bluer, fainter outer halo. There is no apparent spiral structure or prominent dust lanes visible. The overall form suggests a relatively relaxed system without ongoing major mergers, though subtle asymmetries or minor disturbances cannot be ruled out at this resolution. The galaxy appears as an isolated system, without any immediately interacting companions. The observed color suggests it hosts an older stellar population, while the slightly bluer outer regions may indicate ongoing or recent star formation.
