The galaxy appears as a centrally concentrated, elliptical-like structure. Its light profile is smooth with a high degree of central concentration, with a morphology exhibiting a generally rounded shape with subtle isophotal twisting noted in the outer regions. There are no readily apparent spiral arm structures or a distinct disk component that would suggest it to be a spiral galaxy. The overall color of the galaxy leans toward redder hues, transitioning into more yellow tones in the galactic center. This color suggests an older stellar population and potentially lower levels of ongoing star formation. There is no strong indication of active galactic nucleus activity through broad emission lines or unusual colors. The galaxy appears relatively isolated, and without any signs of recent major merger events or strong tidal disturbances.
