The galaxy appears to be a spiral galaxy, observed at an oblique angle, so it appears as an oval shape in the image. The central bulge is a bright yellowish color, indicating an older stellar population, with little to no active star formation in that region. The galaxy disk exhibits hints of spiral arm structure, with a bluer color compared to the central bulge, suggestive of ongoing star formation within these arms. There is a slight asymmetry to the galaxy's structure. No obvious signs of a major ongoing merger are present. The light distribution suggests a substantial, relatively smooth stellar component.
