The galaxy presents an elongated, cigar-shaped morphology. It exhibits a generally smooth appearance, but there are some notable features that suggest possible disturbances. 

The color distribution is not uniform. There is a clear gradient, transitioning from a redder hue at one end to a yellower tone at the other. This suggests varying stellar populations or dust content across the galaxy.

There is a hint of asymmetry or irregularity that suggests that this galaxy may have undergone a minor interaction with another galaxy. The disturbance is not major, but it has clearly affected the galaxy's morphology to some degree. There is no clear sign of merging.
