The galaxy presents as a relatively smooth, elliptical-like object. Its light is centrally concentrated, with a bright core that diminishes gradually towards the outer edges. There is a slight color gradient, shifting from a whiter hue in the center to a more yellowish tone in the outer regions. No prominent spiral arms or distinct dust lanes are observed. The overall structure appears undisturbed, with no apparent signs of a major ongoing merger or tidal disruption. The object displays a generally rounded morphology. Based on its apparent color and smooth structure, the stellar population likely consists of a significant population of older stars.
