The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, centralized bulge with a gradual decline in luminosity towards its outer edges. The galaxy appears to be a relatively isolated system, showing no strong visual signs of on-going major mergers or significant tidal disturbances. It is possible that there are minor disturbances affecting this galaxy. A subtle color gradient is observed, with the central bulge exhibiting a slightly yellower hue compared to the bluer disk, potentially indicating a difference in stellar populations. The galaxy appears to be a relatively massive system.
