The galaxy presents as a spiral type, oriented at a slight incline relative to our line of sight. The central bulge exhibits a moderate size and a yellowish hue, suggesting an older stellar population. Faint spiral arms emanate from the core and extend outwards. A blueish tint can be seen within the arms.

The galaxy’s overall structure indicates a stable, relatively unperturbed system, with no prominent signs of ongoing major mergers or tidal distortions. The morphology suggests an intermediate stage of galactic evolution, where star formation is still occurring within the spiral arms. 
