This galaxy presents as a largely featureless, smooth object. Its light profile suggests a high degree of central concentration, with a radial falloff in surface brightness indicating an elliptical morphology. The dominant color appears yellow to red, suggesting an older stellar population. This older stellar population is also consistent with the galaxy’s relatively smooth appearance, as opposed to a disk structure. While the overall morphology suggests a lack of recent major merger activity or significant star formation, there are some hints of possible minor disturbances or interactions. It appears to be a rather massive galaxy, with considerable luminosity.
