The galaxy presents as a moderately luminous, elliptical system. It exhibits a smooth, relatively featureless morphology with a high degree of central concentration. The shape appears oblate, tending toward an "in-between" elliptical classification, rather than perfectly spherical or highly elongated. The color profile suggests an older stellar population, evidenced by its reddish-yellow hue. There are no visible spiral arms, dust lanes, or other distinct features commonly associated with younger, star-forming galaxies. No signs of major galactic mergers or interactions are visually apparent, although there is a possible hint of minor tidal disturbance in the outskirts.
