The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its color index suggests a population of older stars, resulting in a yellow-reddish hue. There is little evidence of distinct spiral arms or active star formation regions within the observable portion of the galaxy. The overall shape is close to round, with no apparent signs of major disturbances or ongoing merger activity, though a minor disturbance cannot be fully ruled out. Based on the morphology, one may infer that this galaxy has a substantial stellar mass and a relatively low star formation rate.
