The galaxy presents as a slightly inclined disk galaxy. There is a central bulge that appears bright and concentrated, suggesting an older stellar population. The disk exhibits some structure, possibly faint spiral arms or flocculent star formation regions, though the resolution limits a definitive assessment. The color gradient indicates a shift from bluer hues in the outer disk, potentially indicative of ongoing star formation, to redder hues in the bulge, consistent with a population of older, redder stars. The overall morphology suggests a disk galaxy that is neither perfectly smooth nor strongly disturbed. Some asymmetry or minor disturbances in the disk's structure cannot be ruled out based on this image alone, but no major mergers or significant tidal features are apparent.
