The galaxy presents a somewhat elliptical morphology. There appears to be a central bulge region that is relatively smooth and appears brighter, indicating a high concentration of stars. Surrounding the bulge is a fainter, more diffuse disk, suggesting a spiral-type galaxy observed at an oblique angle. The disk displays a blueish tint. The blue color suggests ongoing star formation. There appear to be some distortions in the galaxy's structure, possibly indicative of minor gravitational interactions or disturbances. These disturbances may contribute to the ongoing star formation inferred by the blue color.
