The galaxy presents an apparent irregular morphology. A bright, concentrated central region dominates the structure, possibly indicative of a bulge component. The galaxy exhibits an overall bluish hue in its outer regions, suggesting the presence of younger stellar populations and ongoing star formation. There's a faint hint of possible tidal features or disrupted structure extending from the main body, though the image quality limits definitive classification. Overall, the galaxy appears to be undergoing some form of interaction or disturbance.
