The object appears to be a spiral galaxy viewed at a high inclination. The central bulge is bright and slightly elongated, exhibiting a white-yellow hue indicative of a population of older stars. Evidence of faint, tightly wound spiral arms extends from the bulge, creating a flattened disk-like structure. The arms show some blue color, likely due to ongoing star formation. There are hints of dust lanes visible as dark regions within the disk, especially along the edges. There might be tidal disturbances, as one area has faint hints of an extended region. The galaxy's light distribution is centrally concentrated. There are areas of color distortion that could be imaging artifacts.
