The galaxy presents as a single, luminous object with a pronounced central bulge. The light distribution appears centrally concentrated, with a smooth, elliptical profile. It shows no apparent spiral arm structures or distinct features associated with ongoing major mergers, although the light distribution is not perfectly uniform. The object displays a greenish hue, potentially indicating active star formation, although this needs verification through spectroscopic data. Based on the data provided, the redshift of the galaxy suggests it resides at a significant cosmological distance. Overall, this appears to be a relatively massive galaxy with an intermediate level of star formation activity.
