The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution indicates a high degree of central concentration, with a gradual decline in luminosity outwards from the core. The color profile suggests a population of older stars, with a yellowish hue dominating the central regions. There's little evidence of spiral arm structures or significant dust lanes, supporting the classification as a galaxy with primarily smooth features. It appears as a largely undisturbed system with a well-defined, symmetric shape. There is some evidence of bluer colors in the outer edges, which might be due to younger stars there.
