The galaxy presents as a relatively smooth, centralized structure with a concentrated core. It is roughly elliptical in shape, deviating slightly from a perfect circle, appearing more disc-like. There are faint, diffuse extensions of light surrounding the central core, indicating a halo or outer region. The color gradient suggests that the central region is dominated by older stellar populations, whereas the outer regions are more bluer, indicating there is some star formation present. There is little to no evidence of spiral arm structures or significant dust lanes within the galaxy. No major mergers or tidal disruptions are obvious based on morphology. 
