The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless. It exhibits a high degree of central concentration with the majority of its light emanating from a compact core region. The color profile indicates a bias towards redder wavelengths. There is no clear evidence of spiral arm structures or significant dust lanes. Faint, diffuse extensions surround the main galactic body, potentially indicative of tidal interactions or past merger events, though these features are subtle. The galaxy is observed to be generally round. There is a slight asymmetry visible in the light distribution, potentially suggesting a minor ongoing interaction or internal disturbance. The overall appearance is consistent with an evolved system with subdued star formation activity.
