The galaxy presents as a relatively smooth, elliptical structure. Its morphology is largely spheroid, showing a highly centralized concentration of light intensity that gradually decreases outwards. The color profile suggests an older stellar population, appearing more yellow and red in the central region. There is no distinct spiral arm structure or obvious dust lane features. The galaxy exhibits a seemingly quiescent state with no prominent indications of active star formation regions, which points to a possible lack of cool gas for star forming regions. No obvious tidal features or merging signatures are visible, indicating a gravitationally undisturbed system.
