The galaxy presents as a largely elliptical morphology with a smooth, centrally concentrated luminosity profile. The core exhibits a yellow-orange hue, suggesting a population of older, redder stars dominating this region. This central bulge transitions gradually outward, with a decreasing surface brightness. There is little evidence of spiral arm structure or prominent dust lanes within this galaxy. The galaxy appears to be relatively undisturbed, exhibiting a high degree of symmetry, with no obvious signs of recent or ongoing mergers. The overall color suggests a relatively low rate of star formation compared to bluer, star-forming galaxies.