This galaxy appears to be a disk galaxy, observed at a near edge-on inclination. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Extending outwards is a fainter, bluer disk, indicating regions of ongoing star formation, although appearing overall more muted. There's a hint of asymmetry in the disk structure. The overall morphology suggests it is not undergoing major merger activity, although there might be some minor tidal disturbances or interactions present. Overall, this galaxy displays characteristics between a pure elliptical and a spiral galaxy.
