The galaxy presents as a centrally concentrated system, exhibiting a smooth, elliptical morphology. It appears largely featureless with no apparent spiral arm structure or significant dust lanes visible. The primary color is a yellowish-orange hue, suggesting a dominant population of older stars and a relative lack of ongoing star formation. The galaxy exhibits a high degree of central concentration, with luminosity decreasing gradually from the core towards the outer regions. There is minimal evidence of recent or ongoing merger activity.
