The galaxy appears to be a relatively bright, massive system observed at a redshift of approximately 0.39, suggesting considerable distance. Morphologically, it exhibits a somewhat smooth profile, with a slight elongation or asymmetry rather than a clearly defined disk or spiral structure. The light distribution suggests a centrally concentrated bulge component. There appears to be a slight hint of disturbance or interaction, potentially with smaller companion galaxies. There is a blue coloring on one end which implies recent star formation. Overall, the galaxy is likely an elliptical transitioning from a spiral.
