The observed galaxy presents as a relatively small, elongated object, and is observed to be an unusual green hue. The primary morphology appears smooth and featureless. The smooth light distribution suggests a lack of significant internal structure like spiral arms or dust lanes. The color may indicate active star formation or unusual gas content within the galaxy. There is no obvious evidence of tidal tails, merging features, or other indications of recent or ongoing interactions with other galaxies. A more detailed spectroscopic analysis would be required to further characterize the object.
