The galaxy appears to be a spiral galaxy viewed at a significant angle. It displays a prominent central bulge, exhibiting a yellowish hue indicative of an older stellar population. One side of the spiral structure contains a region with bluer light, suggesting the presence of younger, hotter stars and ongoing star formation. A faint, distorted structure appears connected to the main body, potentially indicating a minor gravitational interaction. There is no obvious indication of a major merger, or grand design spiral arms. The galaxy is neither completely smooth nor highly irregular; rather, it has some features but not well-defined spiral arms.
