This galaxy presents as a relatively smooth, elliptical structure. The light profile is centrally concentrated with a gradual falloff in intensity towards the outer regions. There is a slight blueness to the color, suggesting the presence of some young stars, though it is dominated by older stellar populations. The round morphology indicates little to no disk presence. There is some faint indication of minor disturbances, but the galaxy is mostly undisturbed with no clear signs of any ongoing major merger activity or tidal features.
