The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. The color profile indicates an older stellar population, predominantly yellow with hints of red. There is no clear evidence of spiral arms or significant dust lanes. The galaxy's shape is roughly circular, showing minimal signs of tidal disruption or interaction with other galaxies. There is no obvious active galactic nucleus or intense star-forming regions.
