The galaxy presents a largely smooth morphology. Its overall shape appears elliptical, with a high degree of roundness. The central region exhibits a brighter concentration of light, suggesting a bulge component. There is a subtle indication of bluer colors extending from the center, potentially indicative of some degree of star formation. No significant spiral arm structures or major disturbances are readily apparent in this image. There may be some minor disturbances visible, but mostly looks relatively undisturbed. The galaxy appears to be a relatively isolated system, without signs of a major ongoing merger.
