The galaxy appears to be a spiral galaxy, observed at a near edge-on angle. Prominent spiral arms are visible, exhibiting a blue hue suggestive of active star formation. There is evidence of a central bulge, though it does not appear to dominate the galaxy's overall structure. A subtle bar feature may be present across the central region. The overall morphology suggests a relatively undisturbed system, with no obvious signs of major mergers, although a possible minor interaction or disturbance cannot be ruled out based on the image alone. The galaxy's disk appears relatively smooth, but with significant features that point to underlying spiral structure.
