The galaxy presents as a centrally concentrated, smooth object, exhibiting a near-elliptical morphology. Its core is bright, with a yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient from the center outwards, transitioning to a fainter, slightly bluer periphery. The lack of discernible spiral arms or dust lanes indicates it is likely an early-type galaxy, potentially an elliptical or lenticular galaxy. No significant tidal features or close companion galaxies are apparent, suggesting it is not currently undergoing a major merger event. The galaxy appears relatively undisturbed, with no strong evidence of active star formation within the visible spectrum.
