The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge with a diffuse halo extending outwards. There is little evidence of spiral arm structure or prominent dust lanes. The color profile suggests a population of older stars, with a reddish-yellow hue dominating the galaxy's light. The high degree of roundness suggests it is likely close to an E0 elliptical galaxy type, meaning it has the least amount of ellipticity. There is no strong indication of tidal disturbances or ongoing major mergers.