The galaxy presents a diffuse, oblong morphology. The light distribution suggests a central concentration, though it lacks a clearly defined nucleus. A slight curvature or distortion is apparent in the overall shape, potentially indicative of tidal interactions or an ongoing merger event. Star formation appears to be present throughout the galaxy, as indicated by the blue hue. There is no evidence of well-defined spiral arms or a distinct disk structure. Based on its color and morphology, the galaxy is likely an actively star-forming system undergoing some level of gravitational disturbance.
