The galaxy presents as a largely featureless elliptical system. The light profile is smooth and centrally concentrated, with a gradual fall-off in surface brightness towards the outer regions. Color gradients are subtle, but the core appears to be somewhat yellower, indicating a population of older stars. The outer regions show a slightly bluer tint, suggesting the presence of some younger stars. There is no visible evidence of spiral arms, a bar structure, or significant dust lanes. The galaxy appears relatively undisturbed.
