The galaxy presents a somewhat elongated, cigar-shaped morphology. The central bulge exhibits a smooth, concentrated appearance, appearing nearly spheroidal in shape. Proceeding outward from the core, a disk structure is faintly discernable, exhibiting a gradual decline in surface brightness. The disk component displays hints of warmer hues and less-organized structure, suggesting areas of active star formation. There appear to be some minor gravitational disturbances or tidal features present, suggesting possible past or ongoing interactions with smaller satellite galaxies.
