The galaxy presents as a smooth, elliptical-like structure with a centrally concentrated, bright core. The overall color profile suggests a population of older stars, exhibiting a yellowish-red hue, concentrated towards the center. There is little evidence of spiral arms or significant dust lanes. The light smoothly diffuses from the central bulge outward, with a slight elongation in its shape. Based on the image, star formation appears to be relatively quiescent within the galaxy. There might be signs of minor tidal disturbances.
