The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a smooth morphology, with a high degree of central concentration, indicating a substantial bulge component. The dominant color appears to be a yellowish-orange hue, suggesting an older stellar population with diminished recent star formation. A slight color gradient is observed, with the central region appearing more reddish-orange than the surrounding halo. There is a very slight hint of a possible disk, but it is very subdued. No signs of prominent dust lanes, spiral arms, or ongoing major merger activity are apparent. There is some evidence of a very minor disturbance or tidal feature extending on one side of the galaxy.
