The galaxy appears to be a relatively large, disk-shaped spiral. Its core exhibits a strong concentration of light, appearing yellow-orange in color. The inner regions of the disk are more luminous than the outer ones, and the galaxy's profile suggests it is being viewed at an oblique angle relative to its plane, revealing a somewhat flattened shape. The arms are not sharply defined, displaying a rather smooth, blended distribution of light. There are some subtle hints of bluer regions within the outer disk, indicative of ongoing star formation, although the overall color impression suggests an older stellar population. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or significant tidal interactions.
