This galaxy exhibits a complex morphology, appearing as a likely merging system. The primary component presents a somewhat amorphous shape, lacking a well-defined spiral structure or elliptical profile. There is a noticeable concentration of light towards the core, suggesting the presence of an older stellar population. Fainter, diffuse light extends outwards from this central region. 

A secondary, smaller object is located in close proximity to the primary component. This object appears more compact and distinct, and is slightly offset from the main galaxy. There is potentially some tidal distortion or interaction between the two objects, though it's not definitively clear from the image alone.

Overall, the galaxy displays a moderate blue color, indicating recent or ongoing star formation. Patches of varying color suggest a mix of stellar populations and potentially some dust obscuration. The system is not exceptionally bright, suggesting a moderate luminosity. Further spectroscopic analysis would be needed to confirm the nature of the interaction and star formation activity within this galaxy.
