The galaxy presents an elongated, cigar-like morphology, indicative of an edge-on or highly inclined disk. A central bulge is visible, exhibiting a bright, concentrated luminosity. Moving outward from the bulge, the disk appears relatively smooth, with hints of spiral structure suggested by subtle color variations, particularly bluer regions interspersed within the yellowish-red disk. There appears to be minimal signs of any major ongoing mergers or significant tidal disturbances.
