The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a concentrated, bright yellow-orange hue, suggesting a population of older stars. Moving outward from the center, the color transitions to a slightly bluer and less intense shade, indicating the presence of younger stars within the galactic disk, although their overall contribution is less dominant. There is very little evidence of spiral arms or distinct features, supporting its classification as an elliptical galaxy. Faint irregularities in its outer halo suggest past or ongoing minor gravitational interactions with smaller galaxies or stellar streams. The overall shape is slightly elongated, hinting at a possible deviation from perfect sphericity.
