This galaxy appears as a moderately luminous object with an overall elliptical morphology. There is a slight elongation, and the light profile suggests a smooth distribution without prominent spiral arms or a central bar structure. Color gradients within the galaxy are subtle, suggesting a relatively uniform stellar population. The concentration of light towards the center is apparent, indicating a bulge component, but it is not overly dominant. There are some indications of minor tidal disturbances in the outer regions, but no obvious signs of a major ongoing merger. Given its redshift and apparent magnitude, the galaxy likely resides at a significant cosmological distance. The overall impression is that of a relatively evolved galaxy with moderate stellar mass and a low star formation rate.
