The observed galaxy presents as a relatively smooth, centrally concentrated structure. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light gradually diminishes radially outward, transitioning into a reddish-orange color in the outer regions. Although a prominent disk structure is not immediately apparent, subtle variations in color and luminosity suggest potential underlying features. Some asymmetry is evident, particularly in the distribution of the outer regions, potentially indicative of minor gravitational disturbances. No prominent tidal tails or bridges, characteristic of major merger events, are readily visible. The overall form appears to be somewhere between elliptical and a disk galaxy, with a smooth texture.
