The galaxy presents as a somewhat elongated, likely disk-shaped structure, oriented nearly edge-on from our line of sight. One end of the galaxy appears brighter and bluer, suggesting recent or ongoing star formation activity. This region exhibits a less uniform morphology, possibly indicating the presence of spiral arm fragments.

Moving across the galaxy's body, the light shifts towards redder hues, suggesting an older stellar population. This central area appears smoother, possibly indicative of a bulge component dominated by older stars. The opposite end of the galaxy is significantly less bright and compact, though still with the same redder hue. 

The overall morphology indicates a galaxy that hasn't experienced a major merger event recently. While the morphology is largely smooth, the presence of a bluer and less uniform region at one end hints at some ongoing processes such as star formation. There is possibly a disturbance to the galaxy, but whether that is an artifact or minor merger is still up for investigation.
