The galaxy appears to be a spiral galaxy, observed at an angle somewhere between edge-on and face-on. There is some evidence of disk structure, potentially with spiral arms visible, although the limited resolution makes definitive classification challenging. The galaxy exhibits a central bulge that appears relatively smooth and concentrated, with an apparent redder color than the surrounding disk. The disk shows a bluer hue, suggestive of ongoing star formation. There is an apparent asymmetry in the disk, possibly indicating a minor interaction or disturbance in its recent history. Some regions in the disk show enhanced brightness. The overall morphology suggests a galaxy that is relatively undisturbed and potentially undergoing moderate star formation.
