The galaxy presents a largely smooth, rounded morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a subtle color gradient, with the core exhibiting a yellowish-orange hue, potentially indicating a population of older stars. No distinct spiral arms or prominent features indicative of ongoing star formation are readily apparent. There may be some minimal signs of gravitational disturbance, but it is not a recent major merger. The smooth appearance and lack of features implies it is not a disk galaxy. Overall the morphology points toward an elliptical-type galaxy, with a low star formation rate.
