The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. The color profile suggests a dominant population of older stars, as evidenced by the reddish-yellow hue of the galaxy's core and the more diffuse outer regions. There is no readily apparent disk structure or spiral arm morphology. Evidence for ongoing or recent major merger activity is minimal, with a symmetric light distribution. The light is fainter on the outer edges and brighter towards the center. The roundness of the object suggests minimal distortion due to interactions with other galaxies. There are hints of an underlying blue, which could indicate some star formation is present. The relatively smooth light profile suggests a evolved state.
