The galaxy presents as a moderately luminous object at a redshift of approximately 0.21. Its overall morphology appears to be disturbed, possibly indicative of a recent or ongoing interaction or merger event. The light distribution suggests a complex structure. There is a bright, dominant central region that appears smooth, possibly representing the core of the original galaxy or a coalescing nucleus. Around this central region, there are other bright regions or knots of activity. These structures are separated but appear to be gravitationally bound to the central region.

The presence of these knots suggests regions of heightened star formation. A range of stellar populations seems to be present, with bluer components indicating younger stars. Dust extinction appears moderate overall, contributing to the galaxy's redder hue. There is a hint of tidal features, suggesting potential tidal interactions or recent merger activity. The galaxy's mass is estimated to be significant, consistent with the presence of merging components and active star formation. The star formation rate is elevated, relative to other galaxies of this mass.
