The galaxy presents an overall lenticular morphology, exhibiting a prominent central bulge and a flattened disk. The bulge appears smooth and yellowish, suggesting a population of older stars. The disk component, while relatively smooth, displays a subtle blue hue, hinting at ongoing or recent star formation activity. There are no apparent spiral arms or bar structures visible. No major mergers or tidal disturbances are discernible, though subtle asymmetries in the disk may indicate a minor interaction in the past. The galaxy's redshift suggests it is at a considerable distance. Its angular size appears relatively small, implying a moderate physical size.
