The galaxy appears to be a spiral galaxy, observed at an oblique angle. Two well-defined spiral arms are visible, extending outwards from a central bulge. The spiral arms seem loosely wound. The central bulge exhibits a yellow hue, suggesting an older stellar population. The spiral arms display a bluer color, indicative of ongoing star formation. The galaxy shows no obvious signs of major mergers or significant tidal disturbances. There is a hint of a bar structure in the inner region. Overall, the galaxy presents a classic spiral morphology.
