The galaxy appears to be a spiral, though the image resolution limits a definitive classification. It exhibits a central bulge that is yellow, suggesting an older stellar population. The disk component shows some blue tint, hinting at more recent star formation, although the image is not sharp enough to resolve individual star-forming regions. The galaxy appears moderately inclined to our line of sight, presenting an elliptical shape, and displays no strong signs of recent major mergers. There are hints of slight asymmetry in the outer regions of the disk, which could indicate a minor interaction or internal disturbances.
