The galaxy appears to be a luminous, relatively smooth, elliptical galaxy at a redshift of approximately 0.19, placing it at a considerable distance. Its morphology suggests it is an early-type galaxy dominated by an older stellar population, evident from its yellowish-red color. It is relatively compact, with an estimated effective radius of approximately 5 kiloparsecs. There is no strong evidence of recent or ongoing major merging events. The galaxy's light distribution is centrally concentrated. The galaxy shows a relatively high degree of roundness. Subtle color variations are visible across the galaxy’s profile, possibly indicating variations in metallicity or age of the stellar populations within it.
