The galaxy presents as a spiral structure with a relatively bright central bulge. The spiral arms are prominent, displaying a tightly wound morphology. The arms exhibit distinct blue regions, suggesting active star formation is present. The central bulge shows a yellowish hue, indicating an older stellar population is more dominant in that region. There appears to be a slight inclination of the disk relative to our line of sight. No obvious signs of major mergers or significant tidal disturbances are visible. The galaxy appears relatively isolated, without any immediate companion galaxies. The spiral structure dominates the visible morphology; the bulge is comparatively small.
