The galaxy presents as a centrally concentrated, relatively smooth, and slightly elongated structure. It exhibits a bright, diffuse core that fades into a less defined outer region. There are no obvious spiral arms or distinct features readily apparent. The color appears generally bluish-white, suggesting a moderate amount of ongoing star formation. Faint hints of possible disturbances or minor irregularities are observed, but these do not dominate the overall structure. The overall impression is that of a galaxy transitioning between a disky and elliptical morphology, potentially an early-type spiral or a lenticular galaxy.
