The galaxy appears to be a spiral galaxy, viewed at an oblique angle, exhibiting a flattened disk structure. A central bulge is visible, showing a high concentration of light indicating a substantial population of older stars. The disk component exhibits spiral arm structures. The arms appear somewhat tightly wound. There are hints of dust lanes within the spiral arms. Overall, the light distribution suggests a more or less even stellar population throughout the disk. The galaxy displays a color gradient, with the central bulge exhibiting a yellow-orange hue that transitions to bluer tones in the outer disk, suggesting the presence of younger, hotter stars in those regions.
