The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, appearing brightest at its core and gradually fading outwards. The color gradient suggests a relatively old stellar population dominating the galaxy, indicated by its yellowish hue, particularly within the central region. There is a subtle hint of bluer light in the outer regions which may point to younger stars. There are no prominent spiral arms, bars, or dust lanes visible. The overall shape is predominantly rounded, with no apparent signs of significant tidal distortions or ongoing major merger events. Minor disturbances may be present, but these are not immediately obvious from visual inspection alone.
