The galaxy appears to be an elliptical galaxy. It presents a generally smooth, rounded morphology, lacking a prominent disk or spiral arm structures. The light distribution is centrally concentrated, exhibiting a bright core that gradually fades outwards. The core shows a hint of yellowish color, which may indicate an older stellar population. A faint, diffuse bluish halo surrounds the core, possibly indicating the presence of younger stars and some ongoing star formation, however weak. There is no apparent dust lane or other signs of significant dust obscuration. Overall, the galaxy seems relatively isolated, lacking major signs of tidal disturbance or interaction with nearby galaxies, though a slight disturbance cannot be fully ruled out.
