The galaxy presents as a largely smooth, centrally concentrated object with an approximate redshift of 0.21. It exhibits a predominantly circular morphology with minimal discernible features or disk-like structures. The galaxy's color profile suggests a moderately active star-forming region in the central nucleus, surrounded by an inner disk of what may be older stars. The outer regions of the galaxy are dominated by what appears to be a halo of older stars and dust. There are minimal signs of any recent major mergers, but there are subtle indicators of minor gravitational disturbances or interactions. Overall, the galaxy appears to be a relatively quiescent system with a substantial stellar mass.
