The galaxy presents as an elongated, cigar-shaped structure, likely viewed at a significant inclination. There is a prominent central bulge region exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a more diffuse, bluish disk component, indicative of ongoing star formation. The disk appears relatively smooth, lacking the distinct spiral arm structure often observed in disk galaxies. However, there are subtle color variations across the disk, with bluer regions potentially tracing areas of enhanced star formation. The galaxy appears relatively isolated, showing no strong signs of tidal interactions or major mergers in the immediate vicinity. There is a slight asymmetry in the outer disk, possibly indicating a minor past interaction or internal disturbances.
