The galaxy presents a roughly elliptical morphology, appearing largely smooth in texture with a concentrated central region. Its overall color suggests a slightly redder spectral energy distribution. There is minimal evidence of significant star formation activity within the visible light spectrum. No obvious spiral arm structure or a prominent disk are detectable. Based on the galaxy's shape, and color, and redshift it is a likely candidate for an elliptical galaxy with minimal ongoing star formation. It shows no signs of recent or major merging activity, though there are possibly hints of minor disturbances. The estimated effective radius suggests a physically large galaxy.
