The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a moderate ellipticity, appearing somewhat rounded in shape, but not perfectly spherical. There are no prominent dust lanes, spiral arms, or other features typically associated with disk galaxies. The galaxy's light profile suggests it is mostly composed of older stellar populations, which are likely responsible for its yellowish-white color. There is no strong evidence of ongoing major mergers or tidal disturbances, although subtle irregularities might indicate minor interactions. The galaxy displays a smooth, gradual decline in light intensity from the core outwards.
