The galaxy appears as a centrally concentrated, relatively smooth object. It presents with a nearly circular morphology. A bright, yellowish core dominates the image, suggesting a substantial population of older stars and potentially a supermassive black hole at the galactic center. The surrounding regions exhibit a gradual decline in brightness. There is little indication of significant spiral arm structure or pronounced dust lanes. The overall color profile suggests that star formation activity is low, and that this object is likely an elliptical galaxy. There is a slight hint of very weak disturbances in the outer reaches of the galaxy, this could be evidence of minor gravitational interaction, although further investigation is required.
