The galaxy presents as an elliptical morphology, appearing relatively smooth in structure. The concentration of light suggests a high degree of central mass, likely dominated by older stellar populations, giving off a yellowish hue. There is no observable spiral arm structure. The galaxy is not perfectly spherical, with a hint of elongation along its major axis. There are no signs of active galactic nuclei, major dust lanes, or tidal disturbances suggesting ongoing or recent major merger activity. Slight asymmetry on one side possibly indicates minor gravitational interaction with an unseen companion galaxy. Star formation rate is likely low.
