The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a noticeable radial color gradient, transitioning from a yellowish hue at the core to a redder, fainter halo. The overall structure appears undisturbed, showing no signs of major mergers or tidal features. The galaxy's luminosity profile seems centrally peaked, with a diffuse outer region. Given the apparent color and smooth structure, the galaxy likely consists of an older stellar population, with little ongoing star formation activity.
