The galaxy appears to be a relatively compact system. The central region exhibits a high degree of light concentration, suggesting a prominent bulge or core component. The galaxy appears to be in the green color range indicating a population of stars that are somewhat older. The overall morphology suggests a possible elliptical or lenticular classification, although some subtle irregularities or faint extensions hint at potential past interactions or internal disturbances. These features, if genuine, are not pronounced, implying a system that is relatively settled in its current configuration. Further investigation is needed to determine if the distortions are real features of the galaxy, or just artifacts of the image.
