The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, likely due to a lack of ongoing star formation and an abundance of evolved stars. There is a faint, extended halo surrounding the central region, indicating a diffuse distribution of stars beyond the main body of the galaxy. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated along its major axis. There is no strong evidence of spiral arms or significant dust lanes. There is a slight indication of a minor interaction or disturbance.