The galaxy presents a generally smooth morphology, with a largely featureless appearance. The light distribution suggests it is an elliptical galaxy. The galaxy exhibits a degree of ellipticity, appearing somewhat elongated. The central region is significantly brighter and more concentrated than the outer regions, indicative of a bulge. There are no prominent spiral arms or dust lanes visible in this image. The color profile indicates that the central bulge region is comparatively redder, which may be due to an older stellar population. There is a slight indication of bluer regions at the edge of the disk which may mean there is some star formation occurring. It appears to be relatively isolated, showing no obvious signs of a major ongoing merger event. There is a faint asymmetry which may suggest a recent disturbance.
