The object appears to be a spiral galaxy, viewed at a high inclination, nearly edge-on. It displays a prominent, elongated bulge that appears smoothly distributed and slightly yellowish in color, suggesting an older stellar population. Fainter, bluer light emanates from the extended disk, possibly indicating ongoing star formation within the spiral arms. There is no obvious central bar structure. The galaxy shows no visually significant merger or tidal features. It seems to be a relatively undisturbed system at this point in time. 
