The galaxy presents as a somewhat elongated spheroid, suggestive of an elliptical morphology or a lenticular galaxy viewed at an angle. The central region exhibits a concentrated luminosity profile, appearing yellowish-white, indicating a population of older stars. Moving outward from the core, a diffuse, greenish-blue halo is observed, possibly indicating the presence of younger stars and ongoing star formation. There is a slight asymmetry in the outer regions, with a subtle extension or disturbance visible on one side, hinting at a possible interaction with another galaxy or a minor merger event in its past. The overall appearance suggests a galaxy with a significant mass and a moderate level of recent star formation.
