The galaxy appears to be a disk galaxy, showing a slight bulge and some evidence of spiral arm structure. The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, a bluer tint is visible, potentially indicating more recent star formation activity within the disk. The arms have a flocculent structure with distinct regions that appear knotty with an irregular shape. The arms also show a low surface brightness relative to the bulge. There may be a companion galaxy or tidal disturbance on one side of the galaxy. It seems like a regular galaxy with no major mergers occurring.
