The galaxy presents as a moderately sized object with a redshift indicating a significant distance. The morphology appears complex, exhibiting features suggesting an ongoing interaction or merging event. There are distinct regions of enhanced luminosity, one noticeably elongated, and another more compact and slightly offset. The color profile indicates a population of older stars contributing to a redder overall hue. This suggests the galaxy is massive with an active star-forming region. Evidences point towards a non-relaxed system, as indicated by the disturbed morphology.
