The galaxy appears to be a relatively luminous, elliptical galaxy with a smooth, centrally concentrated morphology. It exhibits a nearly spherical shape, with only a subtle deviation from perfect roundness. The galaxy's color suggests an older stellar population, dominated by redder stars. No distinct spiral arms or prominent dust lanes are visible. The absence of significant blue color suggests a low rate of on-going star formation. There is no evidence of a major merger event, though some minor disturbance cannot be ruled out at this resolution.
