The galaxy presents as a relatively smooth, disk-dominated system with an elongated, cigar-like morphology. A central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The disk component appears to be viewed edge-on, with a subtle color gradient indicating potential variations in stellar populations or dust content across the galactic plane. There is no obvious strong spiral arm structure. It displays no signs of major tidal disturbances or ongoing mergers, although subtle asymmetry in the disk could indicate minor interaction history. Overall, the galaxy appears to be a relatively isolated and well-defined disk galaxy.
