This galaxy appears as a somewhat diffuse and moderately luminous object. Its overall color suggests a population of primarily older stars, with a redder hue dominating. The galaxy exhibits a generally elliptical morphology, with a lack of distinct spiral arm structure. The light distribution appears relatively smooth, lacking any strong central concentration or prominent features that indicate ongoing active star formation or recent mergers. There may be some minor disturbance present in the galaxy's structure. Given its apparent size and redshift, this is likely a moderately massive galaxy with a fairly low rate of star formation. 
