The object appears to be a galaxy exhibiting a complex morphology, possibly indicative of an interaction or merger event. The primary body of the galaxy presents a diffuse, somewhat amorphous structure with an apparent elongation. There is a discernible secondary component or companion galaxy located nearby; a smaller, more compact object. 

The primary galaxy shows little discernible internal structure or spiral arm features. Its light is relatively uniform and there is a high degree of overall smoothness. The color of the primary galaxy is bluer than the secondary, suggesting a younger stellar population. The secondary component is quite compact and its color more closely approaches the redder end of the spectrum.

There may be a tidal bridge or stream of material connecting the two galaxies, which supports the hypothesis that the two objects are in the process of merging. Overall, the system is characterized by a relatively compact size.
