The galaxy presents as a largely featureless, elliptical-like structure with a relatively smooth light distribution. The central region is dominated by a bright, concentrated core, indicating a high density of stars. The light from the central core is yellow, suggestive of an older stellar population. The outer regions show a diffuse, dimmer halo that transitions smoothly from the core. There is a subtle color gradient with the outer regions having a slightly bluer hue than the core. The overall shape is mostly round. There is no discernible evidence of spiral arms, bars, or ongoing major mergers within the observable image data. 
