The galaxy appears to be a mid-sized object at a considerable distance, evidenced by its redshift. Morphologically, it presents with both smooth and featured characteristics, exhibiting a combination of an elliptical and disk-like structure. The galaxy is approximately circular in shape, but shows signs of irregularities. There is evidence of ongoing or recent merger activity, resulting in disturbed features within the main galactic body. The central region is dominated by a yellowish-orange hue, suggestive of an older stellar population, while bluer components are present at the fringes, indicating regions of more recent star formation. Overall, the galaxy displays an intermediate level of star formation activity and a substantial stellar mass.
