The galaxy presents as a lenticular or possibly an edge-on spiral galaxy, displaying a smooth, elongated morphology. A central bulge appears prominent and relatively bright, exhibiting a slightly redder hue, suggesting an older stellar population. Faint blue hues along the edges of the galaxy indicate some level of ongoing star formation, though it appears subdued. The overall structure indicates a system in a transitional phase, potentially evolving from a spiral to an elliptical morphology, or simply a spiral galaxy viewed at an oblique angle. There is no obvious indication of strong tidal interactions or major merger events in its recent history, although some minor disturbances cannot be ruled out based on this image alone.
