This galaxy appears to be a spiral galaxy, viewed at a nearly edge-on inclination. The central bulge is moderately sized and appears relatively bright, with a smooth, concentrated luminosity profile suggesting an older stellar population in this region. Faint traces of spiral arms can be inferred extending outwards from the bulge, predominantly within the main disk. The disk exhibits noticeable color variation, likely indicative of different stellar populations and star formation regions. Blue hues suggest regions of ongoing or recent star formation. There is some subtle evidence of a bar-like structure within the central region, but it is not distinctly prominent. A minor level of asymmetry is observed in the outer regions of the disk, possibly suggesting a weak gravitational interaction or disturbance event. The overall morphology suggests a galaxy that has not experienced a major merger event recently, but may have undergone minor interactions in its history.
