The galaxy presents a generally smooth, elliptical morphology, with a concentrated central bulge that appears slightly offset from a perfect center. There is a subtle disk component that could be present. The light distribution is relatively even, with a gradual decrease in brightness from the core outwards. Color gradients are subtle, transitioning from a yellower core to a slightly bluer outer halo. There are no prominent spiral arms or distinct dust lanes visible in this image, suggesting it may be a relatively evolved system, potentially an elliptical galaxy. There may be a weak interaction occurring with a smaller object, although it could also simply be a background object. There may be some relatively low levels of star formation occurring in this galaxy.