The galaxy appears to be a relatively compact, disk-shaped structure viewed at a moderate inclination. It exhibits a bright, concentrated central bulge or core, suggesting a high stellar density in that region. The outer regions of the disk show some evidence of structure, but the overall appearance is relatively smooth. The galaxy has a slight asymmetry and what appears to be some distortion that may indicate it has undergone a recent minor merger. The colors visible suggest a diverse stellar population, with bluer hues possibly indicating younger, hotter stars. There is a hint of a faint halo or extended structure surrounding the main body of the galaxy. Overall, this galaxy appears to be undergoing some type of disturbance and exhibits a mixture of both smooth and featured morphological characteristics.
